The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a concentrated luminosity, appearing golden in hue, suggesting a high density of older stellar populations. Moving outwards from the core, the light gradually diminishes, with the galaxy fading into the background sky. There appears to be no distinct spiral arm structure or prominent dust lanes. The shape of the galaxy is elongated, exhibiting a moderate ellipticity, without indications of ongoing major merger events or significant tidal disturbances. Overall, the galaxy presents characteristics of a well-defined, early-type galaxy.
