The galaxy presents as a moderately luminous, relatively compact object. Morphologically, it appears to be an elliptical galaxy, exhibiting a smooth, featureless profile. The light distribution suggests a high degree of central concentration, with the core region being significantly brighter than the outer halo. The galaxy displays an overall yellowish-white hue, with a slight elongation along one axis, deviating slightly from a perfectly circular shape. There is no apparent evidence of spiral arms, prominent dust lanes, or ongoing star formation regions. The galaxy's morphology indicates that it is likely a passively evolving system with a substantial population of older stars and a low star formation rate. There are very minor signs of any disruption to the shape, so this galaxy has likely not undergone a major merger in quite some time.
