The galaxy presents as an elliptical morphology, with a smooth and concentrated distribution of light. The core exhibits a bright, yellowish hue, indicating a population of older stars. The galaxy appears moderately elongated, with an approximate major axis of 4.3 kpc. No distinct spiral arms or prominent dust lanes are visible. Faint, diffuse extensions are observed around the central region, hinting at a less concentrated stellar distribution in the outer regions. There is no clear evidence of a recent major merger or significant tidal disturbance. However, there may be a slight asymmetry in the distribution of light, potentially suggesting a minor interaction in the past. The overall color gradient suggests that star formation is largely suppressed, giving way to a dominance of older stellar populations.
