The galaxy presents as a centrally concentrated, smooth object with an elliptical morphology. The core region exhibits a bright, yellowish-white glow, suggesting a significant population of older stars and a lack of prominent dust lanes. The galaxy fades outwards in intensity, and the outer regions appear slightly bluer than the core. This bluer color likely indicates the presence of a younger stellar population in these regions. There is no clear evidence of distinct spiral arms or a well-defined disk structure, and the object's smooth appearance indicates it is either an elliptical galaxy or a lenticular galaxy viewed face-on. I do not observe any indication of ongoing major merger activity or strong tidal features. The galaxy's morphology suggests a relatively evolved system with a quiescent star formation history.
