The galaxy presents as an intermediate system, exhibiting characteristics of both smooth and disk-like morphologies. It appears to have a significant disk component, with the disk oriented somewhat edge-on relative to our line of sight. There appears to be a central bulge, showing a concentrated region of higher luminosity. The overall color profile suggests a mix of stellar populations; the central regions exhibit a yellowish to reddish hue, possibly indicating older stars.

There is evidence of morphological disturbance. The galaxy is not entirely symmetrical, and appears to have asymmetric arm-like or tidal-tail features extending from the main body. These features could be indicative of a past or ongoing minor merger or interaction with a smaller companion galaxy. Although, these could also be internal features, such as from super-winds or other galactic phenomena.

Given the disk prominence and potential for minor interaction, star formation is potentially active within the disk and/or in the asymmetric features, albeit not aggressively so based on the lack of intense blue regions.
