This galaxy exhibits a generally elliptical morphology, with a smooth, centrally concentrated luminosity profile. The core region is noticeably brighter and appears more yellowish in color, suggesting a higher concentration of older stellar populations. There is little evidence of distinct spiral arms or prominent dust lanes within the visible structure, indicating a classification likely along the elliptical sequence. The outer regions of the galaxy appear to fade gradually, lacking sharp boundaries. There may be a subtle degree of flattening, but overall, it retains a relatively rounded appearance. Signs of recent mergers or significant tidal disturbances are absent, with no apparent distortions in its overall shape.
