The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct disk structure. The light distribution suggests a high degree of central concentration, with a bright, luminous core that gradually fades into the outer regions of the galaxy.

The color profile indicates a redder hue overall, particularly toward the central region. The outer regions exhibit a slightly bluer tint, which could signify a younger stellar population compared to the older, redder stars populating the core. However, this blue component is not strongly pronounced, suggesting that the galaxy's overall star formation rate is relatively low.

There are no obvious signs of ongoing merger activity or significant tidal disturbances. The galaxy's symmetrical shape reinforces the impression of a relaxed system that has likely undergone a period of relative quiescence, free from recent major interactions with other galaxies. The light distribution suggests a spherical or slightly flattened shape.
