The galaxy presents as a slightly elongated, disk-shaped structure. The central region exhibits a bright, concentrated luminosity indicative of a prominent galactic bulge. The color of the central bulge appears to be reddish-yellow, possibly suggesting an older stellar population with a lower rate of recent star formation. Fainter, bluer structures are present within the disk, which may indicate active regions of star formation. The overall morphology suggests a spiral or lenticular galaxy viewed at a relatively high inclination. There is a faint hint of a tidal feature or minor disturbance, potentially indicating a past or ongoing interaction with another galaxy.
