The galaxy presents as a relatively smooth, elliptical-like structure. There is a concentrated central bulge that fades gradually into a more diffuse outer region. The light distribution appears quite smooth, lacking prominent spiral arms or distinct features suggestive of active star formation regions within the observed wavelengths. It appears to be in between a round shape and a cigar shape. Overall, the galaxy exhibits a flattened shape, with an observed ellipticity. The galaxy appears to have a slightly offset center, potentially indicating some gravitational disturbance. The color profile is generally consistent across the galaxy, trending toward redder hues with the exclusion of the very center, which trends towards whiter hues. This color profile, along with the smooth light distribution, suggests an older stellar population.
