The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge region that graduates outwards to a less-defined, fainter halo. There appears to be an absence of significant spiral arm structures, with no obvious dust lanes interrupting its smooth appearance.

The color distribution is dominated by warmer hues, suggestive of an older stellar population. This could indicate that star formation is not currently a dominant process, or perhaps is occurring at a reduced rate. While the galaxy is mostly smooth, some slight irregularities or minor disturbances can be observed in its outer regions. The object's overall symmetrical shape appears roughly circular with only slight elongation.
