The galaxy presents as a relatively smooth, elliptical object with an apparent spherical morphology. There is a noticeable concentration of light towards the galactic center, suggesting a dense stellar population in the core. The color gradient indicates a dominant population of older stars, exhibiting a yellowish-red hue, which is characteristic of a lower rate of ongoing star formation. There is no apparent spiral structure or significant dust lanes, which contributes to the galaxy's smooth appearance. The isophotes appear mostly regular and concentric, supporting the classification as an early-type galaxy. There may be a very faint, diffuse halo surrounding the main body, but the data does not provide a clear indication of its extent or properties. There are no signs of any significant tidal disturbances or ongoing mergers.
