The galaxy presents as a relatively smooth, centrally concentrated object. The light distribution appears roughly elliptical, suggesting a classification toward the elliptical end of the Hubble sequence. The color gradient is subtle, with a slightly yellower core region transitioning to bluer outer edges, indicating a potential mix of older stellar populations centrally and younger populations in the outer regions. No distinct spiral arm structure or prominent dust lanes are discernible, reinforcing the impression of a more quiescent, less actively star-forming system. There is no obvious indication of any major merger events or tidal disturbances. The galaxy's profile is relatively compact. Overall, the galaxy's morphology suggests an early-type galaxy with a smooth light distribution and a lack of prominent features associated with active star formation.
