The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The light distribution appears relatively uniform, lacking prominent spiral arms or distinct features. The core exhibits a bright, concentrated luminosity profile, suggesting the presence of a substantial stellar population and potentially an active galactic nucleus. The galaxy displays a moderate degree of roundness in its overall shape, with a slight elongation. There is no clear evidence of ongoing major merger activity or significant tidal disturbances. The color profile indicates a relatively redder spectral energy distribution, consistent with an older stellar population and a low star-formation rate.
