The galaxy appears as a centrally concentrated object with a relatively smooth overall morphology. It exhibits a largely elliptical shape, with only slight deviations from perfect roundness. The color profile suggests a higher concentration of older stellar populations, which is supported by the generally smooth texture and a lack of prominent spiral arms.

A faint bluish-green hue is visible in a thin band across the center, hinting at possible ongoing, albeit subdued, star formation within a disk-like structure embedded within the galaxy. The bulk of the galaxy, however, displays a yellowish tint, indicative of older, redder stars. There's a subtle extension to one side, suggestive of a potential minor tidal disturbance or an interaction with a smaller companion galaxy. There does not appear to be significant evidence of a major merger or a highly disrupted structure.
