The galaxy presents a generally smooth morphology. The light is concentrated towards the center, with a bright, slightly elongated core. There is a gradual decrease in surface brightness moving outward from the core, with no distinct spiral arm structures or prominent dust lanes visible. The color appears to be largely homogenous throughout the galaxy, with a slightly reddish/yellowish hue indicative of an older stellar population. There are no signs of ongoing major merger activity, though the galaxy may show evidence of minor disturbances upon closer inspection. The overall shape is elliptical, but is close to round.
