The galaxy presents a somewhat elongated, cigar-shaped morphology. Its light profile appears relatively smooth, suggesting it is likely an early-type spiral galaxy. The central region exhibits a bright, concentrated core, potentially indicating the presence of an active galactic nucleus (AGN) or a dense stellar population. There is little indication of distinct spiral arm structure or prominent dust lanes. A faint, diffuse halo surrounds the central region, extending further along the major axis. The galaxy exhibits a slight bluish tint in the halo region, possibly indicative of some ongoing star formation, however low levels of star formation. Based on these characteristics, the galaxy appears to be a relatively massive system. There may be a hint of a tidal tail or interaction with another galaxy in the form of a small blue clump nearby.
