This galaxy presents a largely smooth morphology, with an overall elliptical shape, appearing quite rounded. The color profile suggests an older stellar population, displaying a reddish-orange hue concentrated towards the center, which likely indicates a higher density of evolved stars. There appears to be some evidence of possible tidal interactions with another galaxy, as there is evidence of merging with another galaxy and disturbances within its structure. The galaxy is actively forming stars, although at a modest rate given its mass. The overall smooth appearance indicates an early-type morphology, with a relatively high degree of central concentration. 
