The galaxy presents as a largely featureless elliptical system, exhibiting a smooth light profile indicative of an older stellar population. The central bulge dominates the overall structure. There is a slight elongation, with an approximate aspect ratio suggesting it is moderately round rather than highly flattened or cigar-shaped. A subtle color gradient is present, with the core exhibiting a slightly yellower hue, possibly indicating a higher concentration of older, redder stars. There is little evidence of significant ongoing star formation, with no obvious blue regions or dust lanes visible. A fainter, smaller galaxy is visible in the foreground, which might have had some gravitational interaction with it but the primary galaxy looks undisturbed and is not currently undergoing a major merger. The overall appearance suggests a relatively evolved system, likely composed predominantly of older stars and with a low star formation rate.
