This galaxy presents as an elliptical or lenticular type, with a smooth, centrally concentrated luminosity profile. There's an apparent lack of distinct spiral arms or significant dust lanes, which supports the classification of a relatively evolved system. The galaxy exhibits a subtle elongation, appearing somewhat flattened rather than perfectly spherical. The color profile suggests a dominant population of older stars, with a redder hue in the outer regions transitioning to a slightly bluer central region, possibly indicating some residual or ongoing star formation towards the core, albeit at a low rate. There are no obvious signs of major mergers or significant tidal disturbances in the immediate vicinity, though the asymmetry could indicate a minor interaction in its past. The apparent size, combined with its measured redshift, suggests this is a relatively small to medium mass galaxy.
