This galaxy appears to be a relatively large, luminous object, exhibiting a smooth, elliptical morphology. The light distribution is concentrated towards the center, suggesting a prominent bulge. While largely smooth in appearance, there is a subtle hint of a disk component present, though not strongly defined. The galaxy's color profile indicates a population of older stars, particularly in the central region. There is a noticeable lack of distinct spiral arm structures or active star-forming regions. The galaxy is mostly round, with some minor irregularity in shape. There are no visible signs of a major merger event, though the slight asymmetry may indicate past or ongoing minor interactions.
