The galaxy presents as a relatively smooth, elliptical-like structure. The core region exhibits a high degree of central concentration with a bright, near-spherical distribution of light, suggesting an older stellar population. There is a color gradient visible, with the central core appearing slightly bluer than the outer regions, hinting at some level of recent star formation, although limited. No distinct spiral arms or features indicative of significant ongoing star formation are apparent. There are no signs of tidal disturbances or interactions with other galaxies; it seems to be isolated and relaxed. The overall morphology is generally smooth and undisturbed.
