The galaxy presents a generally smooth morphology, appearing largely elliptical in shape. It is elongated, with an intermediate axial ratio, displaying neither perfect roundness nor a highly elongated cigar shape. No prominent features are immediately apparent, with no obvious spiral arms or distinct disk-like structures visible. The light distribution is concentrated towards the center, indicating a likely bulge component. Color gradients suggest a higher concentration of older stars in the central region, exhibiting a yellowish or reddish hue, transitioning toward bluer colors in the outer regions, possibly indicating ongoing, albeit moderate, star formation. There is no visible evidence of major ongoing merger activity or significant tidal disturbances, though there is a faint object in the near vicinity of the galaxy. This morphology suggests the galaxy is in a relatively quiescent state.
