The galaxy appears as a slightly elongated spheroid, indicating a possible elliptical morphology, with a hint of a disk-like structure. The color profile indicates a population of relatively older stars, contributing to the redder hues, but also displays bluer regions, suggestive of ongoing, though perhaps limited, star formation. There is a subtle asymmetry, with a slight extension or tidal feature visible on one side, possibly hinting at a past interaction or minor disturbance event. The galaxy exhibits a relatively smooth overall texture, suggesting the absence of prominent, well-defined spiral arms or significant dust lanes. Based on apparent size and observed characteristics, it can be inferred that this galaxy is a substantial system with ongoing star formation, and potentially a complex history of interactions.
