The galaxy presents a morphology characteristic of a relatively smooth system. It appears as an elliptical galaxy, or potentially a lenticular galaxy viewed close to face-on. The luminosity profile appears to be centrally concentrated, with a gradual decline in brightness towards the outer regions. There is little evidence of spiral arm structure or significant dust lanes. The galaxy exhibits a moderate degree of ellipticity, appearing somewhat flattened rather than perfectly spherical. No signs of ongoing major merger activity or significant tidal disturbances are observed in the immediate vicinity of the galaxy, though there appears to be some minor disturbance. The color index suggests the presence of a moderately old stellar population, with a relatively red appearance. The estimated size of the galaxy is moderately large. 
