The galaxy presents as a relatively compact object with a noticeable central bulge. The light distribution appears somewhat irregular and clumpy, suggesting a possible recent interaction or internal disturbance. Color gradients within the galaxy indicate a radial change in stellar populations, with bluer regions suggesting younger stars and star formation, particularly towards what appear to be the outer edges. The galaxy is clearly not a pure elliptical system. Instead, there is the suggestion of faint, disturbed spiral arms or tidal features, contributing to its non-smooth appearance. The relatively redder color of the central region may indicate the presence of an older stellar population or increased dust extinction.
