The galaxy presents as a centrally concentrated object, exhibiting a largely spheroidal morphology. There is an apparent lack of significant spiral arm structures or prominent dust lanes. The core region displays a bright, yellowish hue, indicative of an older stellar population. Fainter, diffuse emission surrounds the core, extending outwards in a relatively smooth distribution. There may be faint evidence of minor tidal disturbances or interactions with nearby objects. The overall color suggests a quiescent galaxy, with little ongoing star formation.
