The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that graduates into a relatively diffuse halo. The color profile suggests a population of older stars, with a yellow-red hue dominating the galaxy's overall appearance. There is no apparent disk structure or spiral arms. No significant tidal features or signs of recent merger activity are discernible in the immediate vicinity. The galaxy appears relatively isolated, without any apparent interactions with neighboring galaxies.
