The galaxy appears to be an intermediate-type spiral galaxy, possibly somewhere between an Sa and an Sb. It exhibits a prominent, moderately bright central bulge, and fainter spiral arms that are not tightly wound. There is evidence of dust lanes within the arms, though the resolution limits detailed observation.

The galaxy's overall color suggests a relatively older stellar population, but the bluer regions in the disk indicate ongoing star formation. The lack of a strong, dominant spiral structure indicates that the galaxy may have experienced a minor disturbance in its past, though it appears stable at the current time. The galaxy exhibits a noticeable disk component, but the bulge makes up a significant portion of its light.
