The galaxy appears as a relatively compact, elliptical-like structure. Its core is characterized by a bright, yellowish-white concentration of light, suggesting an older stellar population dominating the central region. Moving outward from the core, the luminosity gradually decreases. There is a faint, somewhat diffuse halo extending from the core, exhibiting a bluish hue. This suggests the presence of a small population of younger, hotter stars and perhaps some ongoing, albeit limited, star formation. The overall structure seems undisturbed, showing no obvious signs of a major merger or tidal interactions. It is relatively smooth in appearance, with a lack of prominent spiral arms or distinct features.
