The galaxy presents a generally smooth morphology, with a slightly elongated, cigar-shaped appearance. The central region exhibits a concentration of light, suggesting the presence of a bulge. Moving outward from the core, the light gradually diminishes, indicating a faint disk or halo structure. The galaxy does not show any obvious signs of spiral arms or other distinct features associated with active star formation, and does not show signs of major merging activity. Colors appear redder in the central bulge and become increasingly blue toward the outer regions.
