The galaxy presents as a roughly elliptical structure with a smooth appearance. The core region displays a concentrated luminosity gradient, transitioning into a more diffuse outer halo. The overall color profile appears to be largely red/yellow, possibly indicating an older stellar population with less active star formation. There is minimal evidence of spiral arm structure or significant dust lanes. The galaxy's morphology appears largely undisturbed, with no strong signs of ongoing major mergers or tidal interactions. A slight asymmetry is noted in the light distribution, but is not significant enough to indicate any disruptive event.
