This galaxy exhibits a generally smooth, elliptical morphology. It appears fairly compact, approximately 3 kpc in diameter based on calculations, with a high degree of central concentration. The overall color is yellowish-white, indicating a predominantly older stellar population. There is very little evidence of significant spiral arm structure or dust lanes. A faint, very slight bluer tint is visible in the outer edges, suggestive of a small amount of ongoing star formation, although this appears to be fairly quiescent overall. There is no obvious sign of tidal tails or major morphological disturbances, suggesting it has not undergone any major merger events recently, or is in the very late stages of merging. The galaxy presents as a relatively isolated, evolved system.
