The galaxy presents as a relatively smooth, elliptical form with a high degree of central concentration. The color profile suggests an older stellar population, appearing redder overall with a subtle yellow hue in the core region. There is little evidence of active star formation visible within the galaxy, and there is no clear spiral arm structure. Faint, diffuse extensions may be present, indicating some tidal interaction or past merger event, but this is not definitive based on the image alone. The galaxy displays an intermediate ellipticity, being somewhat flattened. There may be a slight asymmetry to the isophotes, suggesting a mild disturbance in the overall structure of the galaxy.