The galaxy presents as a moderately bright, relatively smooth and concentrated object with a slight ellipticity. The color profile is predominantly yellow-white at the core, suggesting a population of older stars. There is a subtle radial color gradient, with the outer regions appearing somewhat redder, again consistent with an aging stellar population. No distinct spiral arm structures or dust lanes are discernible in this image. The galaxy exhibits a mostly uniform texture, with no obvious signs of recent major merger events or strong tidal disturbances. There might be a very slight asymmetry, potentially indicating a minor interaction, however this could be internal.
