The galaxy presents a generally smooth, elliptical morphology. The light distribution indicates a high degree of central concentration, exhibiting a bright, yellowish core, possibly indicative of an older stellar population. The shape appears mostly round. There is evidence of a possible tidal interaction or merger event occurring, possibly with another galaxy. I observe some distortion and extended faint emission surrounding the main body of the galaxy, suggesting a dynamically disturbed system. The presence of any clear spiral arm structure or a well-defined disk is not readily apparent, although the galaxy is not perfectly spherical.
