The galaxy exhibits a roughly elliptical morphology, though its structure is significantly disrupted. Evidence of tidal interactions is present, suggesting a possible ongoing or recent merger event. A degree of asymmetry can be observed in its outer regions. The galaxy’s color profile indicates a relatively quiescent stellar population, with redder hues dominating. There may be a faint presence of a disk, but the disruption makes it hard to determine. There is potentially some distortion visible in the distribution of light, further suggesting gravitational interactions. Overall, the galaxy's form suggests a dynamic environment experiencing ongoing structural changes.
