The galaxy presents as a relatively compact object, appearing somewhat elliptical in shape with a major axis exceeding its minor axis. The color profile suggests a dominant redder hue with some blue elements, potentially indicative of a mix of older stellar populations and regions of ongoing star formation. There is a subtle hint of asymmetry or irregularity in its structure, which might be a sign of interaction or disturbance, though the primary impression is that of a galaxy in a settled state. The texture is generally smooth, implying a low degree of clumpiness or distinct, bright star-forming regions. The overall light distribution appears concentrated towards the center, indicating a prominent central bulge, but further analysis is needed to accurately characterize its morphological classification.
