The galaxy presents a largely smooth, elliptical morphology, exhibiting a centrally concentrated luminosity profile. The core region displays a bright, yellowish hue, indicative of an older stellar population likely dominated by red giants and other evolved stars. Moving outward from the center, the intensity gradually decreases, forming a diffuse halo. There is very little evidence of spiral arm structure or significant dust lanes, further supporting a classification as an elliptical galaxy. The overall shape is neither perfectly spherical nor elongated but somewhere in between the two. There are no obvious signs of recent or ongoing major merger activity or strong tidal distortions; any disturbances appear to be at most minor. Based on its color and smooth morphology, the galaxy appears to have a relatively low star formation rate compared to actively star-forming galaxies, consistent with a more passively evolving system.
