The observed galaxy appears as a centrally concentrated spheroid with a relatively smooth light distribution. The core exhibits a bright, slightly yellowish hue, suggesting a population of older stars. The isophotes are generally round, but a slight deviation from perfect circularity can be observed. Diffuse light extends outward from the central region, fading into the background sky, with a possible faint arm or tidal tail feature hinting at past or ongoing gravitational interaction in the upper left quadrant of the galaxy. There is a lack of prominent spiral arm structure or distinct dust lanes. Subtle color variations are present within the extended halo, possibly indicating variations in stellar populations or metallicity.
