The galaxy presents as a somewhat diffuse, elliptical structure with a concentrated central bulge. The core exhibits a yellowish-orange hue, possibly indicative of an older stellar population. Moving outward from the core, there appears to be a gradual transition to a bluer color, suggesting the presence of younger, hotter stars in the outer regions. The overall morphology leans towards being relatively smooth, although subtle irregularities are present. There are hints of faint, extended arms or tidal features, suggesting past or ongoing interactions with other galaxies, albeit the primary structure is quite uniform. Star formation appears to be moderate but detectable, with indications of ongoing or recent activity in the outer reaches.