The galaxy presents a generally elliptical morphology. It appears relatively smooth in texture, with a concentrated central bulge. The color profile skews toward the redder end of the spectrum, suggestive of an older stellar population. There's no obvious indication of prominent spiral arms or significant dust lanes. The galaxy seems mostly undisturbed, showing no clear signs of major tidal interactions or ongoing mergers, although subtle indications of minor disturbances cannot be ruled out. The overall shape leans towards a rounder form rather than a highly elongated or cigar-like appearance. The small size suggests a considerable distance.
