The galaxy appears as a centrally concentrated, relatively smooth object with a discernible but not sharply defined edge. Its overall morphology is elliptical, exhibiting a high degree of circularity. A bright, concentrated central bulge is apparent, surrounded by a fainter, more diffuse halo. There is little evidence of spiral arm structure or significant dust lanes. The color profile suggests a higher concentration of bluer, younger stars towards the center, fading to redder hues in the outer regions. The general smooth appearance suggests that the galaxy is an early-type galaxy, with limited ongoing star formation and a dominant population of older stars. Minor disturbances in its overall structure are not obviously discernible, suggesting the galaxy has not recently undergone a major merging event.
