The galaxy presents as a somewhat diffuse object, with a generally elliptical morphology. It exhibits a smooth appearance, lacking prominent spiral arms or a well-defined disk structure. The color profile appears relatively uniform across the galaxy, showing a slightly redder hue, possibly indicative of an older stellar population or the presence of dust. There is no distinct central bulge that is visible. There is no apparent signs of tidal disturbances or merging events, which suggests the galaxy is currently in a relatively quiescent state.
