The galaxy presents as a centrally concentrated, elliptical morphology. It exhibits a smooth, featureless structure with a high degree of symmetry. The color profile indicates a population of older stars, with a redder hue dominating the central region. The galaxy appears moderately luminous, likely indicative of a high stellar mass. There are no visible signs of active star formation or significant dust lanes. A slight asymmetry in the outer regions might suggest a past minor interaction, though the overall structure appears largely undisturbed. The galaxy's round shape suggests it's relatively face-on, or possibly a true elliptical system rather than a spiral viewed at an angle. It appears to be in a relatively isolated environment, lacking any clear signs of ongoing mergers or interactions with other galaxies.
