The galaxy exhibits a generally smooth morphology, with a slight ellipticity. It displays a concentration of light toward the center, suggesting a prominent bulge or core.  The color is relatively uniform, with a subtle shift towards redder hues in the central region, which could be due to older stellar populations dominating in that area. There may be evidence of a faint, diffuse disk component extending outwards, though this is not well-defined. There is a hint of a blue area on the upper edge of the galaxy, which may indicate areas of ongoing star formation. The overall structure suggests a galaxy that is not undergoing significant recent major mergers, though there might be some signs of minor disturbances in the outer regions.
