The galaxy presents a generally smooth appearance, with a slight elongation along its major axis, giving it a somewhat cigar-like shape. The central region exhibits a concentrated, bright core, suggesting a significant concentration of stars and potentially a supermassive black hole. A subtle color gradient is visible, with a yellowish hue dominating the central bulge. Fainter, bluish tinges are present in the outer regions, possibly indicative of younger stellar populations and ongoing star formation, though at a low rate. No distinct spiral arms or prominent dust lanes are apparent. Minor disturbances are possible in the outer halo, though the image is difficult to see any conclusive evidence of a recent merger or interaction.
