The galaxy presents as a slightly elongated, disk-shaped structure viewed at an oblique angle. A central bulge dominates the visual appearance, exhibiting a concentrated luminosity gradient. The bulge appears to be a yellowish hue, indicating an older stellar population. Surrounding the bulge is a fainter, more diffuse disk, possibly containing spiral arms or other structures, though resolution limits detailed observation. The color of this disk is bluish, suggesting the presence of younger, hotter stars and ongoing star formation, though this appears to be relatively low. The galaxy does not show obvious signs of major mergers or strong tidal distortions, but faint disturbances are possible, which can be further investigated. The overall morphology of the galaxy appears relatively smooth, with some possible features.
