The galaxy presents a moderately inclined disk morphology. It exhibits a bright, yellowish central bulge region, which appears relatively smooth. The disk shows some indications of spiral structure, with faint, greenish arms extending outwards. The arms are somewhat diffuse, suggesting a moderate level of ongoing star formation. There is a notable redder region offset from the bulge, potentially indicative of a region of significant dust obscuration or a distinct population of older stars. Overall, the galaxy's features suggest an intermediate stage of morphological evolution, possibly a spiral galaxy exhibiting characteristics of both early- and late-type systems.
