The galaxy presents as a moderately luminous object, likely a spiral galaxy seen at an oblique angle. The central bulge appears a yellowish hue, indicative of an older stellar population. Fainter spiral arms extend outwards from the core region, displaying a slightly bluer tint, suggesting ongoing star formation within the arms. The galaxy exhibits a generally elongated shape, with a minor degree of irregularity in its structure. A low-level of recent or ongoing interaction with another galaxy is possible, as evidenced by subtle morphological distortions.
