This galaxy exhibits a disk-like morphology, viewed nearly edge-on from our vantage point. The central region is characterized by a bright, concentrated bulge exhibiting a smooth distribution of light. The bulge appears to be ellipsoidal. The galaxy's disk appears thin and elongated, displaying a relatively uniform yellowish color profile. The lack of distinct spiral arm structures suggests a smoother distribution of stellar populations within the disk. There are no obvious signs of a recent major merger event based on visual inspection of the morphology; however, there are minor indications of possible disturbances. The overall color suggests an older stellar population and relatively low current star formation activity. The galaxy appears moderately large in size.
