The galaxy presents an overall smooth, elliptical morphology. The central region exhibits a higher concentration of luminosity, appearing as a bright, slightly elongated core. This core gradually fades outward into a diffuse halo. The color profile suggests a concentration of older stellar populations, with a general lack of prominent spiral arm structures or significant dust lanes. There appears to be a subtle blueish hue suggesting at least some low-level ongoing star formation, although the dominant color is consistent with a passively evolving system. The axial ratio indicates a moderate ellipticity, deviating noticeably from a perfectly spherical shape. There is no obvious evidence of major mergers or significant tidal disturbances in the immediate vicinity of the galaxy.
