The galaxy presents a relatively smooth, elliptical morphology with a concentrated central bulge. There is no prominent disk structure visible. The core exhibits a yellowish-orange hue, suggesting a population of older stars. A faint, diffuse halo surrounds the central region, fading into the background sky. There is no indication of spiral arms, bars, or significant dust lanes. Overall, the galaxy appears to be an early-type system with minimal ongoing star formation, displaying a spheroidal shape that is quite round. There is no clear evidence of any major or minor merging events, though subtle disturbances cannot be ruled out.
