The galaxy presents as a relatively smooth, elliptical structure. Its overall shape is elongated, appearing cigar-shaped when viewed from our perspective. The central region exhibits a concentrated, bright core, likely indicating a high density of stars. Moving outward from the center, the light gradually diminishes. There appears to be a subtle color gradient, with the core leaning towards a slightly redder hue and the outer edges displaying hints of bluer tones, suggestive of a small amount of on-going star formation at the galaxy's edge. There is no sign of any major mergers or dramatic disturbances in the galaxy's structure, though some faint asymmetry may be present at the very edges of the galaxy.
