The galaxy presents as a centrally concentrated object with a generally smooth, elliptical morphology. There is a bright, condensed core region exhibiting a yellowish hue, suggesting an older stellar population. The outer regions display a gradual decrease in surface brightness, transitioning to a more diffuse and bluish color profile. This may be a result of a more sparse distribution of younger stars in the outer regions. The galaxy appears relatively isolated with no major signs of tidal distortion or ongoing merger activity. The object is consistent with an early-type galaxy such as an elliptical or lenticular, viewed close to face-on. Overall, the galaxy exhibits a well-defined, relaxed structure.
