The galaxy appears as an elongated, yellowish structure, suggesting a possible elliptical or lenticular morphology. The galaxy presents a smooth profile, indicative of a lack of prominent spiral arms or dust lanes. It exhibits a relatively concentrated central bulge. There is a slight asymmetry in the distribution of light, hinting at possible interactions or internal disturbances, although no clear signs of tidal tails or merging companions are evident in this image. The overall color suggests a population of older stars, which is consistent with a low star formation rate.
