The galaxy presents as an elongated, elliptical structure. The central region exhibits a concentrated brightness, appearing yellowish-white, suggesting an older stellar population dominating the core. Moving outward from the core, the light gradually diminishes, forming a more diffuse halo. The edges of the galaxy lack distinct spiral arm features and appear generally smooth. The color gradient indicates a potential transition from older, redder stars in the core to slightly younger, bluer populations in the outer regions, although this color difference is subtle. There is no obvious evidence of significant dust lanes or active star-forming regions within the visible structure. The overall morphology is consistent with a relatively massive, evolved system. There may be some indication of mild tidal disturbances, but the galaxy appears largely undisturbed.
