The galaxy presents as a relatively compact, elliptical-like structure. The light distribution appears largely smooth, with a concentration toward the central region, suggesting an older stellar population. There may be a hint of a slight disk component or spiral arm, however they are only very faintly visible. The overall color of the galaxy appears reddish-yellow, which is consistent with a population of older, redder stars and potentially a low rate of ongoing star formation. There is no obvious evidence of a recent major merger event in the image, but there is some minor irregularity, possibly due to a small merger in the recent past. The approximate size of the galaxy appears consistent with typical galaxies in the local universe.
