The observed galaxy presents as an elliptical morphology, with a moderately bright core region that suggests a high stellar density. The galaxy exhibits a relatively smooth luminosity profile, with a gradual decrease in brightness from the center outwards. The overall shape approximates an elongated spheroid. There are no apparent spiral arms or prominent dust lanes visible. A subtle distortion or disturbance may be present along one edge, suggesting a possible minor gravitational interaction. The galaxy exhibits a color gradient, with the core appearing relatively blue compared to the outer regions, potentially indicating differences in stellar populations or dust obscuration.
