The galaxy presents as a moderately sized system, characterized by a predominantly smooth morphology. There is a subtle, yet discernable disk-like component. The galaxy's shape is somewhat elongated, deviating slightly from a perfectly circular profile, trending towards an intermediate classification. The central bulge region appears bright and concentrated, suggesting a significant stellar density. Faint, diffuse features may indicate subtle disturbances, but no major mergers or significant tidal interactions are evident. The overall color profile suggests a mix of stellar populations, with a possible dominance of older stars. The system appears to be undergoing moderate star formation.
