The galaxy presents as a relatively compact, well-defined structure with a smooth central bulge. It exhibits a distinct, flattened disk component, viewed at a shallow inclination. Star formation is clearly evident within the disk, characterized by the presence of localized regions of intense blue emission, suggestive of ongoing or recent bursts of star formation. The galaxy displays an overall organized spiral structure. There are faint indications of potential disturbances within the galaxy structure, possibly suggestive of minor interactions or internal dynamics at play. The galaxy's morphology is intermediate between elliptical and spiral.
