The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears elliptical, exhibiting a largely spheroidal shape with minimal apparent disk structure. The light distribution shows a gradual decline in intensity moving outwards from the core, suggesting a lack of distinct spiral arms or features. There is a subtle color gradient, with the central region appearing whiter or slightly bluer relative to the outer regions, which possess a redder hue. This could indicate a difference in stellar populations, with younger, hotter stars dominating the central regions and older, cooler stars more prevalent in the outskirts. The lack of significant disturbances in its morphology suggests this galaxy has not experienced a recent major merger event. It appears relatively isolated and undisturbed.
