This galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. The core region appears bright and slightly elongated. Moving outward from the center, there is a gradual decrease in luminosity. The galaxy lacks any distinct spiral arm features or prominent dust lanes. The color profile suggests a generally older stellar population, with a hint of blue color within the inner region. There is no indication of any significant tidal disruption or ongoing major merger activity, though there may be evidence of a very minor disturbance in the outer regions. The galaxy appears to be intermediate in roundness, tending closer to a circular shape. Overall, this galaxy is likely a massive elliptical galaxy exhibiting signs of slow or absent star formation.
