The galaxy presents a primarily smooth morphology, suggesting an elliptical classification is likely. There's a subtle hint of a disk-like structure, though it is not a prominent feature. The galaxy appears relatively round in shape, with a slight deviation toward an elongated form. The light distribution is concentrated, with a bright central region. There is no obvious indication of any major merging activity. The color profile shows a redder hue, indicative of an older stellar population, and a suppressed star formation rate.
