The galaxy presents as a centrally concentrated object, with a high degree of overall smoothness and roundness. There is a distinct lack of resolved spiral arm structure or prominent features indicative of ongoing major mergers. The light profile suggests a possible elliptical or lenticular morphology. The observed color appears relatively consistent, with a slightly redder hue. Based on the observed characteristics, there is a suggestion of a passive or quiescent stellar population with little to no actively ongoing star formation. There may be minor disturbances.
