The galaxy exhibits an overall elongated, cigar-shaped morphology. Its central region appears to have a high concentration of stellar mass, indicated by the brighter, yellowish-white light. The outer regions display a bluer hue, suggesting the presence of younger stellar populations and ongoing star formation, albeit at a relatively low rate. This galaxy appears to be relatively isolated, with no obvious signs of major tidal disturbances or ongoing mergers, although a minor disturbance cannot be completely ruled out given the data. The overall structure is relatively smooth, with some hint of faint, diffuse disk-like features. Its overall shape is best characterized as an elongated elliptical galaxy with some star formation.
