The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The core exhibits a yellow-orange hue, suggestive of an older stellar population. The isophotes are generally smooth and concentric, with a slight deviation towards a more elongated, yet not quite cigar-shaped, form. There is a faint, diffuse halo of bluer light surrounding the central region, possibly indicative of some recent, low-level star formation activity in the outer regions. No distinct spiral arms or bar structures are readily apparent. There is no obvious indication of ongoing major mergers, but a few faint irregularities in the outer halo suggest possible minor interactions or tidal disturbances.
