The observed galaxy presents an elongated, cigar-shaped morphology. Its light profile suggests a centrally concentrated bulge that fades gradually outward. The central region exhibits a yellowish hue, potentially indicative of an older stellar population. The outer regions appear bluer, suggesting the presence of younger stars and possibly ongoing star formation. There is no prominent spiral arm structure or distinct bar visible. There appears to be some evidence of a faint dust lane along the major axis that may partially obscure the core. Overall, the galaxy appears relatively undisturbed, showing no major signs of tidal interactions or recent mergers, though there are signs of a small disturbance.
