The galaxy presents as an elliptical morphology, exhibiting a smooth, symmetrical profile with no discernible spiral arms or bar structure. The light distribution appears relatively uniform, concentrated towards the galactic center, with a gradual decrease in intensity towards the outer edges. Its color index indicates a population of older stars, with a yellowish-red hue dominating the visual spectrum. The galaxy is moderately sized, suggesting an intermediate mass range compared to other galaxies. There is no evidence of significant dust lanes or active star formation regions based on the lack of blue light. The overall appearance suggests a passively evolving galaxy with a relatively quiescent history. Faint indications of possible tidal features extending outward may suggest minor past interactions, though no major merger events are clearly evident.
