The galaxy presents as a largely smooth, centrally concentrated object. Its morphology appears elliptical, with an approximate major axis twice the length of its minor axis. The central region exhibits a bright, unresolved core, likely indicating a high stellar density or an active galactic nucleus. Moving outward from the core, the light intensity decreases gradually. The color appears to be trending towards redder hues, which suggests an older stellar population. There is little evidence of spiral arms or significant dust lanes. The galaxy's structure is largely undisturbed, with no obvious signs of ongoing or recent major mergers. Faint extensions, potentially a stellar halo or tidal features, may be present at the extreme edges of the galaxy, however, the image resolution makes it difficult to confirm their presence. Overall, the galaxy's morphology is consistent with a massive, evolved system.
