The galaxy presents as a well-defined elliptical structure. Its core exhibits a bright, concentrated luminosity, suggesting a significant stellar population density and possibly an active galactic nucleus, though higher resolution data would be needed to confirm this. Moving outward from the core, the luminosity gradually decreases, forming a smooth halo around the central region. The overall shape appears somewhat flattened, with a major-to-minor axis ratio of approximately 0.75, indicating a degree of ellipticity. There is faint evidence of a disk structure, though it is not the dominant morphology. The color profile shows a generally redder hue, indicative of an older stellar population with less ongoing star formation. No distinct spiral arms or prominent dust lanes are immediately apparent in this view. Subtle irregularities in the outer regions could suggest past interactions or minor disturbances, but further analysis would be necessary to determine their origin.
