The galaxy presents as a relatively smooth, elliptical structure with a bright central bulge. There is little evidence of spiral arms or a well-defined disk. The light distribution appears concentrated towards the center, gradually fading outwards into a less dense halo. The overall color is indicative of a population of older stars, with a noticeable absence of significant blue star formation regions. Subtle color variations exist, with a slightly bluer hue in the outer regions, suggesting the presence of some younger stars or ongoing, though relatively low, star formation activity. The general morphology aligns with an early-type galaxy, most likely an elliptical or lenticular galaxy. There is no obvious sign of any major ongoing merger events or tidal disturbances. Overall, the galaxy has a regular, undisturbed appearance.
