The galaxy presents as a centrally concentrated object with a roughly elliptical morphology. The core exhibits a bright, yellowish-white hue, suggestive of a population of older stars. Moving outward from the core, there's a gradual transition to a reddish halo or bulge, potentially indicating a mix of intermediate-age and older stellar populations. There is little evidence of spiral arm structure or significant dust lanes, implying a smoother overall distribution of light. The faintness of the outer regions suggests a quiescent star formation rate. There appears to be little evidence of ongoing or recent major mergers or tidal disturbances.
