The galaxy presents as a slightly elongated, likely lenticular, system. It exhibits a bright, concentrated central bulge with a yellowish hue, suggestive of an older stellar population. Extending outward from the bulge is a fainter, relatively smooth disk. There is subtle bluer emission in the disk regions, perhaps indicating some ongoing low-level star formation, but overall, star formation appears quiescent. The galaxy's shape suggests it is viewed at a significant inclination to our line of sight. There is no clear indication of significant tidal disturbances or major merging activity.
