The observed galaxy exhibits a flattened, elliptical morphology, appearing as a smooth, elongated structure in the image. Its color profile suggests a dominant population of older stars, indicated by the central yellowish-orange hue. The lack of distinct spiral arms or prominent dust lanes points towards a relatively quiescent galaxy, likely with a lower rate of ongoing star formation. There is only a hint of blue around the edges. The overall smooth appearance and lack of significant disturbances suggest it is not undergoing any major merging events, and appears well settled. The galaxy displays a moderate level of concentration of light towards its center. The edges are relatively indistinct and fuzzy.
