The galaxy presents a distinct disk-like morphology, viewed at an intermediate inclination relative to our line of sight. There is evidence of spiral arm structure, with flocculent arms emanating from a central bulge region. The bulge appears moderate in size and exhibits a smooth texture, suggesting an older stellar population. A subtle bar-like feature is visible extending through the central region. There is some visual evidence of morphological disturbance in the disk, perhaps indicating a minor interaction or past merger event. The disk component shows a range of colors, with bluer regions likely indicating areas of active star formation. Overall, the galaxy appears to be a spiral galaxy undergoing potentially a minor disturbance.
