The galaxy appears as a somewhat elongated, centrally concentrated object. Its color profile suggests a dominant population of older stars, with a yellowish hue concentrated towards the core. Fainter, bluer, diffuse regions extend outwards from the central bulge, hinting at potential areas of more recent, albeit limited, star formation activity. There are no obvious spiral arm structures or strong signs of a well-defined disk. A slight asymmetry in the outer regions suggests a possible tidal interaction or past minor merger event, although the overall morphology remains relatively undisturbed. The galaxy presents as a moderately massive system, based on its luminosity and size estimates.
