The galaxy presents as a slightly elongated, lenticular or possibly spiral structure, viewed at an oblique angle. There's a subtle concentration of light toward the center, suggesting a nascent bulge. Faint spiral arms may be present, though not well-defined. A blue hue is detectable within the disk, indicative of some ongoing, though potentially low, levels of star formation. Overall, the galaxy appears relatively smooth, suggesting an evolved stellar population. Evidence of any major mergers or significant disturbances are not readily apparent, though a possible minor disturbance could be present. It is a moderately sized galaxy.
