The galaxy appears to be an elliptical type, characterized by a smooth, relatively featureless light distribution. It exhibits a prominent bulge, elongated in shape, with a cigar-like morphology. The color profile suggests a dominant population of older stars, with a subtle redder hue concentrated towards the central region. There is no clear evidence of spiral arm structure or significant dust lanes. The galaxy appears relatively undisturbed, with no obvious signs of ongoing major merger activity or strong tidal distortions, although there is the possibility of minor disturbances. Based on its apparent size and morphology, it is likely a massive galaxy with ongoing star formation.
