The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge. The light distribution suggests a fairly symmetrical structure, with a gradual decrease in brightness moving outward from the core. There is little evidence of spiral arms or significant dust lanes. The galaxy's color suggests a population of older stars and limited ongoing star formation, with a possible redder hue towards the central regions. There are no obvious signs of interaction with neighboring galaxies or major disturbances within the galaxy's morphology. It displays an overall round shape.
