The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless, with a centrally concentrated luminosity profile. The central region exhibits a brighter, bluer hue, suggesting the presence of a younger stellar population or possible active galactic nucleus activity, although further spectral analysis would be required to confirm this. Moving outwards, the galaxy’s color becomes slightly redder and the luminosity decreases gradually, indicating an older, more evolved stellar population in the outer regions. There is no clear evidence of spiral arms, bars, or significant dust lanes. The galaxy does not appear to be undergoing any major merger activity, although there are some very minor disturbances in the evenness of the light surrounding it. The overall shape appears to be more in between round and cigar shaped.
