The galaxy appears as a primarily smooth, elliptical structure. It presents an overall orange-red hue, suggesting an older stellar population with lower rates of current star formation. The galaxy exhibits a relatively symmetrical profile, with a slightly elongated shape, falling between round and cigar-shaped. No strong signs of tidal disturbances or ongoing major mergers are readily apparent, though a subtle asymmetry hints at the possibility of a past or minor interaction. The central region of the galaxy appears brighter and more concentrated, indicative of a substantial galactic nucleus. A faint, diffuse halo or envelope of lower surface brightness is visible surrounding the core, indicating a spheroidal distribution of stars.
