The galaxy presents a largely smooth morphology with a slight ellipticity. Its color profile suggests a relatively evolved stellar population, exhibiting a redder hue in the central bulge region. There appears to be a faint disk component, contributing a subtle blue-ish tint in the outer regions, indicating some level of recent star formation. There are no strong signs of spiral arms or a distinct bar structure. There is one nearby object with an elongated profile that may or may not be interacting with the galaxy. The galaxy's overall appearance suggests a transition state, possibly between a spiral and an elliptical, with a dominant bulge and fading disk features. Based on the apparent roundness, the galaxy is likely viewed at an intermediate inclination angle, not quite face-on nor edge-on. There does not appear to be any indication of a major ongoing merger.
