This galaxy appears to be an elliptical type, exhibiting a largely smooth, featureless morphology. There is a concentrated central bulge that graduates outward in luminosity. The overall shape seems to be somewhere between round and elongated, but is primarily round.

The color profile indicates an older stellar population, shown by a strong presence of redder and yellow wavelengths dominating the galaxy's color profile, particularly at the central bulge. There is still some blue light, indicating that there is still star formation occurring in the galaxy.

There is no apparent evidence of spiral arms or a distinct disk. The lack of dust lanes further supports the classification of the galaxy as an elliptical.

There does not seem to be any other significant structures disrupting its form. There is no sign of tidal tails or distortions, suggesting that the galaxy is not undergoing a major merger, though a minor disturbance or interaction can not be ruled out.
