The galaxy presents a largely smooth, elliptical morphology. It appears moderately luminous, with a concentrated central bulge and a diffuse, fainter halo. The color profile suggests a relatively older stellar population, exhibiting a redder hue in the outer regions and a slightly bluer tinge toward the core. The galaxy's shape is somewhere between round and elongated, with no apparent signs of spiral arms or a prominent disk structure. There is little indication of ongoing major merger events, but some subtle asymmetries may suggest minor past interactions or disturbances. Star formation appears to be minimal.
