The galaxy presents as a somewhat elliptical, though not perfectly round, structure. Its core exhibits a significantly brighter, more concentrated luminosity, suggesting a higher density of stars and potentially the presence of an active galactic nucleus. A noticeable disturbance is apparent in the form of extended features. One component appears as a bright, distinct region, potentially a satellite galaxy undergoing a merger or tidal interaction. Another separate region is a smaller, distinct area. These features introduce an asymmetry to the overall galactic shape. The dominant color is a yellowish-orange hue, which indicates an older stellar population, with a possible lack of significant ongoing star formation. Overall, the galaxy appears to be in an interaction or merging phase, leading to a complex and disturbed morphology.
