The galaxy appears to be an elliptical type, exhibiting a generally smooth and rounded morphology. It presents with a dominant central bulge, characterized by a concentrated, high-intensity glow. The light profile suggests a centrally concentrated stellar population. There appears to be little to no discernible disk component or spiral arm structure. A very slight asymmetry may indicate a minor tidal disturbance or interaction, though no major merger event is evident. The galaxy's color leans towards the redder end of the spectrum, indicating a population dominated by older stars and a low rate of ongoing star formation. It appears to be a relatively massive system.
