The galaxy presents as a relatively smooth, concentrated object with an apparent spheroidal morphology. The central region exhibits a bright, yellowish-white luminosity, suggesting a concentration of older stellar populations. Progressing outward, the light gradually diminishes in intensity. There is little evidence of distinct spiral arm structures or prominent dust lanes. The galaxy's overall shape is close to circular, with minimal observable distortion or elongation. Faint, diffuse extensions are potentially present, though not clearly defined. Interactions with neighboring objects are not apparent.
