The galaxy presents a somewhat diffuse, elongated morphology, appearing neither perfectly elliptical nor distinctly spiral. It is oriented with its major axis approximately vertically in the image.

The central region appears brighter and more concentrated, suggesting a bulge component. The color of the central bulge leans towards yellow.

Moving outward from the center, the galaxy exhibits a bluer hue. This suggests the presence of younger stellar populations and ongoing star formation within the disk. The blue color appears less intense and somewhat patchy, and the overall star formation rate is likely not exceptionally high.

There is evidence of some structural irregularities or disturbances, potentially indicating minor gravitational interactions or past mergers. The galaxy doesn't appear perfectly smooth, and there may be faint tidal features.

The galaxy has an estimated size of several kiloparsecs.
