The galaxy presents as a somewhat elongated, elliptical form. Its light profile appears smooth, lacking prominent spiral arms or distinct morphological features. The color distribution shows a central concentration of yellowish light, suggesting an older stellar population dominates the core. Moving outward from the center, the color shifts to a slightly bluer hue, possibly indicating the presence of younger stars or regions of ongoing star formation, albeit at a low rate. There is a subtle asymmetry in the galaxy's overall shape, with one end appearing slightly more extended than the other. This mild distortion might indicate a past or ongoing interaction with a smaller galaxy, or possibly a tidal disturbance. There is no strong evidence of a major merger event. The galaxy displays a relatively compact size, giving its classification as a likely low-mass galaxy.
