The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in brightness towards the outer regions. The galaxy appears moderately elongated with a major axis to minor axis ratio greater than 2:1. No distinct spiral arm structures or strong dust lanes are discernible in the image. A color gradient appears subtly bluer towards the central region, possibly indicating ongoing or recent star formation, while the outer regions tend toward redder hues, suggestive of older stellar populations. There is no apparent evidence of major tidal disturbances or interactions with other galaxies. Slight visual irregularity suggests possible minor disturbance in morphology.
