The galaxy presents as a flattened, elliptical structure. The central region exhibits a concentrated, yellowish hue, suggesting a bulge dominated by older stellar populations. Moving outward from the center, the color gradually fades, indicative of decreasing stellar density. No distinct spiral arms or prominent dust lanes are discernible within the observed morphology. The galaxy appears relatively smooth in texture, with only a slight degree of irregularity in its overall shape, hinting at a possible minor interaction or internal disturbance. There is no evidence of a bright, active galactic nucleus. Overall, the galaxy appears to be a relatively evolved system, likely exhibiting a moderate stellar mass and a low specific star formation rate.
