The galaxy presents as a spiral galaxy, although its disk is not perfectly defined. It exhibits a bright, yellowish central bulge, indicative of an older stellar population. Surrounding the bulge, the disk component appears bluer, suggesting the presence of younger, hotter stars and ongoing star formation. The galaxy's disk is not observed face-on, but rather at a moderate inclination. This perspective allows for a partial view of spiral arm structure, which appears somewhat flocculent. A distinct feature is visible extending from the main galactic body. This may be indicative of a tidal tail resulting from a past or ongoing interaction with another galaxy, or could be a detached portion of a spiral arm. The galaxy does not appear particularly disturbed in its morphology, despite this feature.
