The galaxy appears to be a relatively smooth, elliptical-type galaxy with a concentrated central bulge. It exhibits an overall rounded morphology, lacking any obvious spiral arm structures or a well-defined disk. The galaxy presents a yellowish-red hue, suggesting an older stellar population, implying that active star formation is suppressed. There are no obvious signs of tidal disturbances, major mergers, or interactions with other galaxies in its vicinity. The structure seems undisturbed. The galaxy's light profile appears relatively even, diminishing gradually outward from the central core.
