The galaxy presents as a single, relatively smooth object with a concentrated central bulge. Its morphology appears to be elliptical, exhibiting a radial distribution of light intensity that peaks sharply towards the core. There is little evidence of spiral arms or other disk-like structures. The galaxy displays a yellowish hue, potentially indicating a population of older, redder stars. The surrounding halo is faint and appears relatively diffuse. There are no obvious signs of ongoing major mergers or tidal disturbances. A slight elongation is observed with the major axis running roughly vertically. The light is moderately concentrated. The overall smooth appearance suggests a system where star formation is suppressed.
