This galaxy exhibits a relatively smooth morphology, suggesting an elliptical or lenticular classification. The central region displays a concentrated luminosity with a yellowish hue, potentially indicating an older stellar population. The overall shape appears to be somewhat flattened, deviating from a perfect sphere. Faint extensions or diffuse features are subtly visible surrounding the central region which could be stellar halos. Based on the apparent lack of defined spiral arms or a prominent dust lane, star formation activity is likely low. There is no indication of significant tidal disturbances or merging events in the immediate vicinity. 
