The galaxy exhibits a generally elliptical morphology, with a bright, concentrated core region. The luminosity appears to diminish gradually from the center outwards, forming a diffuse halo. The galaxy displays a slight elongation, departing somewhat from a perfectly circular shape. There is evidence of a smoother, more homogenous distribution of light, suggesting a lack of prominent spiral arm structures or significant dust lanes. The color profile is primarily redder, which could indicate a population dominated by older stars and a lower rate of ongoing star formation within the visible portion of the galaxy. Overall, the galaxy's appearance suggests characteristics consistent with an elliptical or lenticular type galaxy, with signs of potentially minimal current star formation activity.
