The galaxy appears to be an elliptical galaxy with a smooth, symmetrical morphology. It exhibits a concentrated central bulge that transitions smoothly into the outer regions. There is little evidence of spiral arms or significant dust lanes. The color profile suggests a dominant population of older stars, indicated by the yellowish hue of the central region, with a bluer, younger population in the outer regions. The galaxy shows no signs of ongoing major mergers or tidal disturbances, based on its regular shape and the absence of extended tidal tails or asymmetries. The luminosity profile decreases gradually from the center outwards, consistent with a relatively relaxed stellar distribution.
