The galaxy presents an elliptical morphology. A smooth light distribution is observed across the main body of the galaxy, with no evident spiral arms or distinct features. The central region exhibits a concentrated, bright core, suggesting a possible bulge. The ellipticity of the galaxy suggests a deviation from a perfectly circular shape, appearing somewhat elongated, possibly cigar shaped. There is a subtle suggestion of minor disturbances or tidal features that might be hints of past interactions, although a merger appears unlikely based on the overall regular structure. The color gradients indicate the presence of older stellar populations within the central region.
