The galaxy appears as a centrally concentrated, somewhat spheroidal object with an overall smooth appearance. The core region exhibits a yellowish-white hue, suggesting an older stellar population and relatively low star formation rate within the nucleus. The outer regions of the galaxy present a bluer tint compared to the core, indicative of the presence of younger, hotter stars, and potential ongoing star formation in the disk or outer regions. There is a slight indication of a disk-like structure. No pronounced spiral arms or bars are visible in this image. The galaxy does not show obvious signs of major merging activity or significant tidal disturbances based on this image alone. The light distribution appears relatively regular and symmetric, with a smooth transition in brightness from the core to the outer edges.
