The galaxy appears as an elliptical or lenticular type, characterized by a smooth, centrally concentrated luminosity profile. There is a noticeable lack of defined spiral arms or prominent dust lanes. The central region exhibits a bright, concentrated core, likely indicative of an older stellar population. The galaxy exhibits a slightly yellowish-white hue, suggesting a relatively low rate of ongoing star formation. The overall morphology implies a system with a high degree of internal order and a significant spheroidal component. There might be a very subtle, diffuse disk component but its presence is uncertain. The galaxy appears generally undisturbed.