The galaxy presents an elliptical morphology, appearing generally smooth with a dominant central bulge. There is a slightly disturbed feature or possible merging event occuring at the top of the galaxy, with a possible tidal tail structure. The distribution of light is centrally concentrated, with a noticeable decrease in surface brightness moving outward. The colour profile reveals a redder core, indicative of an older stellar population, with bluer hues in the outer regions suggestive of more recent star formation activity. There is no apparent spiral arm structure. The galaxy appears relatively isolated.
