The galaxy presents as a relatively compact object, exhibiting a primarily smooth morphology. A central, bright region dominates the galaxy's structure, appearing nearly spheroidal with a high surface brightness, indicative of a dense stellar population or an active galactic nucleus. Surrounding the central region is a fainter, disk-like component, possibly displaying some degree of structure. The overall color profile suggests the presence of both older stellar populations, evidenced by reddish hues, and regions of recent or ongoing star formation, highlighted by bluer colors. There is no clear indication of a major merger event in progress, although there might be some subtle asymmetry suggesting a minor disturbance. The galaxy is not perfectly isolated, suggesting the potential for future interactions with neighboring galaxies, even though there are no obvious tidal features. The absence of strong spiral arm structures or a highly irregular morphology supports a classification as an elliptical or lenticular galaxy.
