The galaxy appears to be a smooth, elliptical or lenticular type, exhibiting a concentrated central bulge that dominates its overall structure. The light distribution is relatively even, with a gradual decrease in intensity from the core outwards. There's a noticeable lack of distinct spiral arms or prominent dust lanes, suggesting a population of older stars and a low rate of current star formation. The galaxy exhibits an orange-red hue, indicative of an aging stellar population. The overall morphology appears undisturbed, lacking signs of any ongoing major mergers or significant tidal interactions with other galaxies. There might be a very faint, diffuse halo surrounding the central region, but it is barely discernible.
