The galaxy presents a primarily elliptical morphology, exhibiting a smooth, concentrated central bulge. The light distribution appears relatively uniform throughout the galaxy, without prominent spiral arms or distinct substructures. The galaxy exhibits an overall yellowish hue, possibly indicating an older stellar population with less ongoing star formation, with some suggestion of a subtle disk-like component surrounding the central bulge. There may be evidence of a slight tidal disturbance or interaction. The galaxy is nearly face-on and possesses a slightly elongated shape, with an approximate axis ratio of 0.96.
