The galaxy presents a predominantly smooth morphology, lacking a prominent disk structure. The light distribution appears centrally concentrated with a high degree of radial symmetry, exhibiting a near-circular projected shape. There is a slight deviation from perfect ellipticity, but no apparent bar or spiral arm features are visible. The galaxy's color profile suggests a generally older stellar population with a subtle color gradient toward the center. No significant signs of tidal disturbances or ongoing major mergers are observed, although a faint, unresolved asymmetry could potentially indicate a minor interaction in its recent history. Overall, the galaxy appears to be a relatively quiescent system.
