The galaxy appears as a moderately luminous object, exhibiting a generally elliptical morphology. It is roughly 3.9 kpc across, located at a redshift of approximately 0.065. A dominant, smooth bulge is visible within the central region, surrounded by a faint disk. The disk structure presents a slightly mottled texture. The light from the galaxy suggests a population of intermediate to old stars, with some ongoing, but relatively low star formation. There is a notable absence of strong spiral arm features or significant dust lanes. The galaxy shows no obvious signs of recent major merger activity, though there might be some subtle asymmetry or minor disturbances within the disk region that could suggest minor interaction.
