The galaxy presents an overall smooth appearance with a centrally concentrated bulge. The color profile suggests an older stellar population, with a dominant yellowish-orange hue, particularly within the central region. There is a subtle, diffuse bluer component extending outward from the central region, potentially indicating some ongoing, albeit low-level, star formation. The galaxy exhibits a moderate ellipticity, appearing somewhat elongated rather than perfectly spherical. There are indications of gravitational interactions or disturbances based on the asymmetrical features, with possible faint tidal features or minor distortions visible. These disturbances may be indicative of a past or ongoing merger event.
