The galaxy presents as an elliptical morphology with a notably smooth profile. A prominent, bright central bulge dominates the light distribution. The light tapers off gradually towards the edges, lacking sharp boundaries. Its overall shape is elongated, with a relatively high degree of ellipticity, resembling a cigar shape. Subtle color variations are observed, with a central yellowish hue transitioning to slightly bluer tints in the outer regions, indicating some ongoing, though perhaps limited, star formation. No clear spiral arms or bar structures are discernible within this resolution. There is no clear evidence of ongoing merging activity or major disturbances in its overall structure. The galaxy's stellar mass is substantial, classifying it as a mature and evolved system.
