The galaxy appears to be elliptical in morphology, displaying a smooth, centrally concentrated light profile. There is a distinct lack of spiral arm structures or significant dust lanes visible in this image. The galaxy presents a generally rounded shape, with a minor deviation towards an elongated form. The central bulge exhibits a brighter, yellowish hue, suggesting an older stellar population. Fainter, bluer light is observed in the outer regions of the galaxy indicating the presence of ongoing, but relatively low, star formation. No signs of major mergers or significant tidal disturbances are immediately apparent, although a possible minor asymmetry is detectable. The overall impression is of a relatively quiescent galaxy.
