The galaxy presents as a relatively smooth, centrally concentrated object with a high degree of symmetry. It appears elliptical in shape, exhibiting a predominantly round morphology with a lack of any discernable spiral arm structure or strong bar features. There is a clear, bright core, suggesting a concentration of stellar mass. The color profile indicates a yellowish hue towards the center, potentially indicative of an older stellar population. The outer regions of the galaxy appear fainter with a slightly bluer color, implying a possibility of some ongoing, but relatively low, levels of star formation. No strong tidal features or indications of recent major mergers are readily apparent, although there's a slight irregularity in its outer regions.
