The galaxy presents as a smooth, elliptical morphology. It exhibits a concentrated central bulge, with light gradually diminishing towards the outer regions. The galaxy appears to be of a moderate size and has a yellow-white hue, suggesting an older stellar population. The isophotes show an elliptical shape, with no significant distortions, tidal tails, or evidence of recent merger activity observed. There are no prominent spiral arm structures or dust lanes visible. The galaxy appears relatively isolated in its immediate vicinity.
