The galaxy presents as a relatively small, elliptical system, likely several kiloparsecs in effective radius. Its color is predominantly yellow/red, suggesting an older stellar population with minimal ongoing star formation. The morphology appears generally smooth, lacking distinct spiral arm structures or prominent dust lanes. There is a slight elongation to the galaxy's shape, deviating from a perfectly circular profile; however, the smoothness suggests it is not currently undergoing a major merger. There may be evidence of a minor tidal interaction or past merger event considering the subtle disturbances in its otherwise undisturbed shape. The galaxy exhibits a degree of central concentration, with a brighter core fading outwards. Overall, the observed characteristics are consistent with an evolved galaxy with a dominant spheroidal component.
