The galaxy appears to be a relatively smooth, elliptical system. It exhibits a high degree of central concentration with a bright, diffuse core. There's a noticeable falloff in luminosity moving outward from the center, and a generally rounded morphology is observed. No distinct spiral arm structures or prominent dust lanes are apparent. The overall color profile indicates a lack of significant ongoing star formation, suggesting an older stellar population. There is no obvious evidence of any major mergers or tidal disturbances affecting the galaxy's structure. Faint extensions of light are possibly present.
