The galaxy presents a largely smooth morphology, appearing elliptical in shape rather than displaying prominent spiral arms or a distinct disk structure. The light distribution suggests a central concentration, with a bright, compact core gradually fading into the outer regions. Color gradients are subtle, showing a tendency toward redder hues in the core compared to the slightly bluer outskirts. There is little evidence of significant dust lanes or recent major merger activity disrupting the overall symmetry. The galaxy appears relatively undisturbed.
