The galaxy presents a somewhat amorphous morphology. The central region exhibits a high surface brightness, appearing as a bright, concentrated core. There are faint, diffuse extensions surrounding the core, appearing slightly asymmetric. A subtle distortion or tidal feature may be present, indicating a possible past or ongoing interaction. Color gradients are observable, with the core appearing bluer than the outer regions, suggesting differing stellar populations. Overall, the galaxy appears relatively compact. The overall structure does not show a distinct spiral arm pattern, and is characterized by a general lack of defined features.
