The galaxy presents a largely smooth morphology, with a concentrated central bulge. The overall shape appears to be elliptical, trending towards a more rounded appearance, with only a slight elongation observed. There's no distinct spiral arm structure visible. The color profile suggests a population of older stars, as indicated by the yellowish-red hue concentrated in the core. There's no indication of significant ongoing star formation, with only subtle blueish regions visible in the outer regions. The system doesn't seem to be undergoing any major mergers or significant disturbances based on the overall structure.