The galaxy presents a generally smooth, elliptical appearance. It exhibits a high degree of central concentration, with the light intensity decreasing gradually outwards. The galaxy appears to be fairly massive. There is a possible slight distortion in the galaxy's morphology and some indications of merging activity or tidal interactions. No distinct spiral arms are visible. The galaxy displays a reddish hue, suggesting a population of older stars and a relatively low rate of star formation. It is moderately luminous. It has an inclination close to face-on.
