The galaxy presents a generally smooth, elliptical morphology with a notable central bulge. The light distribution is concentrated towards the core, exhibiting a radial gradient in brightness. The primary color appears yellowish-white in the central region, possibly indicating a population of older stars. There is a slight elongation to the galaxy's shape, with a hint of a disk-like structure or tidal disturbance, as evidenced by some faint features extending from the main body. There may be subtle variations in color or texture, but no distinct spiral arms or prominent star-forming regions are clearly discernible at this resolution. The galaxy seems to have intermediate mass and relatively low star formation rate. Evidence does not strongly suggest an ongoing major merger, though some minor disturbances cannot be ruled out.
