The galaxy presents as a concentrated elliptical-like structure, exhibiting a generally smooth morphology. The light distribution appears relatively even across the galaxy's body, lacking prominent spiral arms or a pronounced central bulge. It seems moderately compact, with a discernible but not extremely sharp edge. There appears to be a slight elongation in its shape. The color profile suggests an older stellar population, with a yellow to red hue, indicating less ongoing star formation activity. There's also a faint, diffuse halo surrounding the central region. Possible minor disturbances in its structure suggest a history of gravitational interactions, but no major mergers or significant tidal features are immediately apparent.
