The object appears to be a spiral galaxy viewed at an oblique angle, not quite face-on. The disk exhibits a degree of visible structure, suggestive of prominent spiral arms. The galaxy presents a central bulge that is moderately sized relative to the overall disk. The spiral arms are relatively tightly wound. The color profile suggests that the galaxy is moderately evolved, with a significant population of older stars, but with ongoing star formation. There is no evidence of significant tidal disruption, suggesting that the galaxy has not recently undergone a major merger. There's no obvious visual indication of a strong bar structure bisecting the central bulge, although a weaker bar structure is not ruled out.
