The galaxy presents an elliptical morphology, appearing elongated with a high degree of axial ratio. The central region exhibits a concentrated and relatively smooth luminosity profile, suggesting a significant stellar population and potentially a central supermassive black hole. The color appears generally reddish-yellow, indicative of an older stellar population, although there may be subtle variations in color across the galaxy's extent, indicating variations in stellar populations or dust content. The overall structure appears largely undisturbed, with no clear evidence of ongoing major mergers or tidal interactions. Faint hints of diffuse emission extend outwards from the main body of the galaxy.
