The galaxy presents a generally smooth morphology. The central region exhibits a concentrated luminosity with a yellowish-white hue, potentially indicating an older stellar population. Surrounding the core, there's an extended, diffuse greenish emission, possibly indicative of ongoing star formation or ionized gas. The overall shape appears somewhat rounded. There might be some minor tidal disturbances or faint structures present within the galaxy's halo, although the image resolution makes it difficult to discern details.
