The galaxy presents as an elliptical morphology, displaying a smooth, diffuse structure with a concentrated central bulge. The light distribution appears relatively uniform, lacking prominent spiral arms or significant dust lanes. There's a subtle color gradient, with the central region exhibiting a yellowish hue, suggesting an older stellar population. Moving outward from the core, the galaxy transitions to a slightly bluer tint, indicative of more recent star formation activity or a younger population. The overall shape deviates slightly from a perfect circle, hinting at a mildly elongated or ellipsoidal form. There might be evidence of a very minor disturbance or tidal interaction based on slight asymmetry in the outer regions, although the galaxy overall appears to be in a relatively quiescent state.
