The galaxy presents an apparent angular size indicative of a moderately distant object. The light profile suggests a morphology that may be transitioning between elliptical and disk-like. A dominant central bulge appears prominent, exhibiting a yellowish hue. The overall structure is elongated, possibly cigar-shaped, though the image resolution limits precise determination. Hints of spiral arm structures are visible in the bluer light distribution.

Disturbances or interactions are potentially present. Patches of bluer light are visible, indicating regions of active star formation. Some asymmetrical light distribution may be present, suggesting a minor interaction, merger, or some other disturbance of the system. 