The galaxy presents as a relatively smooth, elliptical-like structure with a slightly elongated shape. The central region exhibits a bright, concentrated core, suggestive of a high stellar density. The color profile appears to shift from a yellowish hue in the core to a slightly redder tint toward the outer regions, possibly indicating a shift in stellar populations with older, redder stars dominating the periphery. There is a suggestion of a faint disk-like structure extending horizontally. Overall, the galaxy exhibits minimal signs of significant recent merger activity or major disturbances. There is little to no dust observed.
