The galaxy appears to be an early-type spiral, showing a notable bulge component, and a fainter disk component. The central region is bright and elliptical in shape, indicating a substantial population of older stars. The disk presents a bluer hue, potentially suggesting ongoing star formation. The spiral arms appear tightly wound and faint.

The galaxy's overall structure is relatively smooth, but there appears to be some minor morphological distortion that could suggest a past or ongoing interaction with a smaller galaxy, although no signs of a merging partner are visible in this image. The galaxy appears to be moderately massive, suggesting a reasonably high luminosity.
