The galaxy presents a largely smooth morphology with a centrally concentrated luminosity profile. The galaxy's overall shape appears somewhat elliptical, leaning toward a rounded form, although it is neither perfectly spherical nor highly elongated. Faint hints of a disk-like structure are perceptible, though not sharply defined.

The color gradient suggests a population of older stars, particularly toward the galactic center, with light trending towards redder wavelengths. An absence of significant dust lanes or prominent star-forming regions is noted, which is further evidenced by the galaxy's color, suggesting lower rates of ongoing star formation activity. There are no obvious signs of ongoing or recent major mergers or strong tidal disturbances. However, minor asymmetric features might suggest possible past interactions or minor disturbances.
