The galaxy exhibits a morphology consistent with a spiral galaxy viewed at an oblique angle. A central bulge appears prominent, displaying a yellowish hue, suggestive of an older stellar population. Fainter, bluish regions extend from the central bulge, possibly indicating the presence of spiral arms and younger, hotter stars. The shape of the galaxy appears somewhat elongated. There is no obvious sign of strong ongoing star formation activity, such as bright HII regions. The galaxy does not present any obvious signs of major mergers or strong tidal disturbances.
