The galaxy presents as a generally smooth, elliptical morphology. It exhibits a bright, concentrated core region with a yellowish hue, possibly indicating an older stellar population and minimal ongoing star formation. The outer regions of the galaxy appear slightly more diffuse, fading smoothly into the background. There is no evidence of strong spiral arm structure or a prominent disk. Faint, blue-ish regions appear within the galaxy, potentially indicating regions of active star formation, despite their minimal visual prominence. There is an object to the northeast of the galaxy that could either be gravitationally associated with the main galaxy or a chance alignment. This secondary object is noticeably more compact and yellow in color. There is not significant visible distortion in the overall shape, suggesting no major ongoing merger events.
