The galaxy presents an elliptical morphology, displaying a smooth, centrally concentrated light distribution. The central region exhibits a bright, yellowish-white core, suggesting a higher density of older stellar populations or the presence of an active galactic nucleus, although no distinct features indicating AGN activity are immediately apparent from the image alone.

Moving outwards from the core, the color shifts towards a bluer hue, indicating the presence of younger, hotter stars within the galaxy's disk or outer regions. The galaxy appears somewhat elongated, with an apparent tilt relative to the observer's line of sight.

There's a subtle asymmetry to the galaxy's overall structure. While broadly elliptical, a slight distortion or extension is observed on one side, possibly indicative of a minor gravitational interaction or recent merger event. The overall appearance suggests a galaxy undergoing a transition, evolving from a more irregular or disk-dominated system towards a smoother, spheroidal form. Star formation appears present throughout the galaxy.
