The galaxy presents with a predominantly smooth morphology. Its overall shape is largely elliptical, appearing nearly circular with a slight deviation towards an elongated form. The light distribution is centrally concentrated, exhibiting a bright, unresolved core that gradually fades outwards. The central region shows a bluish hue, suggesting the presence of hotter, younger stars, or a possible active galactic nucleus. A faint reddish structure is seen extending from the core, indicating a region of possible dust absorption or a faint stellar population. There appears to be some degree of disturbance or asymmetry present in the overall structure, possibly indicating a recent or ongoing minor interaction or merging event.
