The galaxy presents a generally smooth, elliptical morphology. A concentrated central bulge region is evident, exhibiting a reddish hue, potentially indicative of an older stellar population or significant dust obscuration. Surrounding this central region is a more diffuse halo, appearing greenish-white, suggestive of ongoing star formation and/or a population of younger, hotter stars. The overall shape is slightly elongated. There appears to be a minor asymmetry or disturbance in the outer regions, possibly indicating a past or ongoing interaction with another galaxy. The galaxy displays a relatively compact size and does not exhibit any prominent spiral arms or well-defined disk structures. There is a suggestion of minor tidal features.
