The galaxy presents an elliptical morphology with a smooth, largely featureless appearance, indicative of an early-type galaxy. The light distribution is concentrated towards the center, showing a gradual decrease in intensity outwards. Its color profile leans towards the redder end of the spectrum, suggesting a stellar population dominated by older, redder stars, and a relatively low rate of ongoing star formation. The galaxy appears to be undergoing, or to have undergone, minor gravitational interaction with a smaller, bluer object located nearby. The primary galaxy exhibits a slight distortion in shape, potentially due to tidal forces. While a dominant smooth component exists, there is a subtle indication of disturbance, potentially related to interactions with the companion galaxy.
