The galaxy presents as a single, diffuse object with a notably ellipsoidal morphology, exhibiting a smooth light distribution. Its color index suggests a population of older stars, imparting a reddish-yellow hue. Within the overall structure, two brighter, distinct regions are observed, indicating either active galactic nuclei or regions of intense star formation obscured by dust. There appears to be an interaction occurring, or perhaps recent interaction, given the disturbed morphology and non-uniform light distribution. There is a possibility of ongoing or recent merger event. The galaxy appears relatively isolated.
