The galaxy appears to be a lenticular or early-type spiral galaxy, viewed at an oblique angle. It exhibits a relatively smooth, centrally concentrated light distribution, suggesting an older stellar population. The central bulge is prominent and displays a yellowish hue, indicative of evolved stars. There is a faint, flattened disk component extending outward from the bulge, showing a slightly bluer color than the core. The galaxy appears to be mostly unperturbed, with no obvious signs of recent major mergers or tidal interactions, though a slight asymmetry or minor disturbance cannot be ruled out entirely. The overall shape is elongated, tending toward a somewhat cigar-like form.
