The galaxy presents as a relatively compact object with a slightly elongated morphology. The color profile suggests a population of both older, redder stars and younger, bluer stars, with the redder components potentially more concentrated towards the galactic center, though the blending of light makes it difficult to be certain. There is some evidence of faint, diffuse light extending beyond the core, possibly indicative of a stellar halo or tidal features. There is not any indication of a spiral arm structure nor any well-defined disk component. The irregularity may be indicative of minor disturbances or interactions. The general appearance is of a galaxy that is undergoing, or has recently undergone, some form of interaction or has undergone some form of evolution.
