The galaxy presents a generally smooth, elliptical morphology. The core exhibits a bright, concentrated luminosity with a yellow-orange hue, likely indicative of an older stellar population. The isophotes appear to be largely circular, indicating minimal distortion due to tidal interactions or recent mergers. Faint, diffuse light extends outwards from the central region, gradually fading into the background. There is very little evidence of spiral arms or dust lanes. Overall, it appears to be a fairly well-formed, undisturbed galaxy.
