The galaxy appears as a relatively smooth, centrally concentrated object. There is some indication of a faint, extended halo or disk structure around the central bulge. The light distribution seems fairly uniform, with no obvious spiral arm features or prominent dust lanes visible in this image. The overall shape appears somewhat elliptical, tending toward round, rather than highly elongated. No major signs of ongoing merger activity or strong tidal disturbances are immediately apparent, although there may be subtle indications of minor interactions. The color suggests a moderate population of older stars and possibly ongoing, but not extremely vigorous, star formation.
