This galaxy presents as a moderately bright, lenticular system with a smooth, elliptical morphology. The central bulge appears prominent and exhibits a yellowish hue, indicative of an older stellar population. Moving outward from the core, a diffuse disk is observed, which appears slightly bluer than the bulge, suggesting the presence of some younger stars and possibly ongoing, but low, star formation. There is no apparent spiral structure, nor are there any signs of significant tidal disturbances or mergers visible. The galaxy's overall appearance indicates it is a relatively evolved system.
