The galaxy appears as a centrally concentrated object with an overall smooth morphology. The light distribution is centrally peaked, suggesting a significant bulge component. The galaxy exhibits a nearly circular appearance, indicating a round morphology, with no obvious signs of a disk structure. There is no evidence of any major mergers or significant tidal disturbances in the immediate vicinity of the galaxy. The color profile appears relatively uniform across the galaxy, with a slightly yellowish hue indicative of an older stellar population.
