The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. There is a notable lack of defined spiral arm structures or prominent dust lanes. The color profile suggests a relatively older stellar population, with a slight shift towards redder wavelengths. The overall structure appears undisturbed, with no obvious signs of ongoing major mergers or tidal interactions, though there might be some minor disturbances in the outer regions, given its classification. The round shape suggests it is seen nearly face on. The galaxy displays a relatively compact core, with a gradual decrease in luminosity towards the outer regions.
