The galaxy presents an elliptical morphology, appearing elongated with a cigar-like shape. The central region is dominated by a concentrated, luminous core, suggesting a high density of stars. A gradual decline in brightness extends outwards from the center, with the light distribution appearing relatively smooth and diffuse. There is a subtle color gradient observed, with a tendency toward redder hues in the central regions, potentially indicating an older stellar population. Fainter, bluer regions are observed in the extended areas of the galaxy, possibly indicative of some ongoing, albeit low-level, star formation. No prominent spiral arms or distinct features are apparent, indicating a relatively quiescent morphology. There is no readily apparent evidence of major mergers or significant tidal disturbances affecting the galaxy's structure.
