The galaxy presents as a concentrated central bulge surrounded by a fainter, more diffuse halo or disk. The central region exhibits a smooth texture, with a near-spherical morphology. I detect what appears to be the beginning of a disk like structure. The light distribution suggests that the disk component is not very well defined. There is a slight possibility of a tidal interaction, but it would be extremely minor. Redder colors appear concentrated in the central bulge, possibly indicating an older stellar population, while the outer regions show bluer hues, which may signify younger stars, or recent star formation. The overall structure indicates that it has not undergone a recent major merger event. There is no visual evidence of significant dust lanes or other complex morphological features within the galaxy.
