The galaxy presents as a single, relatively smooth object with a noticeable central bulge. The light is concentrated toward the center, indicating a high stellar density in the core region. The color appears somewhat yellow, suggesting a population of older stars. There is little evidence of prominent spiral arms or significant dust lanes. The overall shape is elliptical or spheroidal, displaying high rotational symmetry. There's a faint hint of bluer light at the periphery, which could indicate some ongoing, albeit low-level, star formation. The galaxy does not appear to be undergoing any major merging events or significant tidal disruptions based on its morphology.
