The galaxy presents as a somewhat smooth, centrally concentrated object. The light profile appears relatively symmetrical, suggesting a lack of significant ongoing major merger activity or strong tidal distortions. There is faint, diffuse material extending outward from the central region. Visually, there is a hint of a disk, but a significant portion of the light is concentrated in a bright, unresolved core. The color is primarily a yellowish-white, with a slight bluing towards the outer edges. This suggests the presence of a relatively older stellar population in the core, with possibly younger, bluer stars contributing to the outer regions, indicating moderate levels of star formation. The overall morphology appears somewhat rounded, rather than elongated or cigar-shaped. There may be very minor disturbances or faint features, but the dominant impression is of a relatively undisturbed system.
