The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge. The overall shape is generally round, displaying a slight elongation rather than a highly flattened disc. The galaxy exhibits a color gradient, transitioning from a bright, almost white core to a bluer hue in the outer regions. This color variation may imply ongoing, albeit moderate, star formation activity. Subtle structural irregularities or minor disturbances are present, suggesting potential interactions or past mergers. Despite these hints of activity, the galaxy maintains a generally relaxed and quiescent appearance.
