The galaxy presents a generally smooth, elliptical morphology. It exhibits a bright, concentrated core region that gradually diffuses outwards into a less defined halo. The color profile is dominated by yellow and red hues, suggesting a relatively older stellar population. There are hints of a faint, extended envelope surrounding the main body of the galaxy, though this is not clearly resolved. No distinct spiral arm structures or prominent dust lanes are visible. The galaxy appears largely undisturbed, with no obvious signs of a major ongoing merger event. There is slight asymmetry in the outer region of the halo indicating a possible minor interaction with a smaller galaxy.
