The galaxy presents a roughly elliptical morphology, with a smooth, diffuse appearance dominating its overall structure. There is a slight elongation. Some signs of internal structure are visible. The primary body appears undisturbed; however, it is interacting with another galactic body. Evidence of a merging event or tidal interaction is suspected, potentially with a nearby companion. The color distribution suggests a mixed stellar population, with a gradient from more yellowish hues in the central region to slightly bluer tones in the outer areas. This may indicate older stars concentrated in the core and younger stars in the disk or arms. Overall, the galaxy exhibits characteristics consistent with a massive system undergoing a period of interaction, showing evidence of both a relatively relaxed, evolved component and potentially ongoing star formation activity.
