The galaxy presents as a lenticular-type morphology, appearing as a relatively smooth, disk-like structure with a lack of prominent spiral arms. It has a pronounced central bulge that dominates the galaxy's overall luminosity. The bulge exhibits a yellowish hue, suggesting an older stellar population. The disk component appears flattened, viewed at a shallow inclination. The color gradient transitioning from the bulge to the outer disk is subtle, with the disk maintaining a similar yellowish-white color. No significant dust lanes or prominent star-forming regions are readily apparent within the disk, indicating a relatively quiescent state of star formation. The galaxy does not appear to be strongly interacting or merging with any neighboring galaxies, and shows no obvious tidal features. The morphology is predominantly smooth, with a higher concentration of light in the central regions and a gradual decrease towards the edges. Overall, the galaxy has a well-defined structure but lacks any major distinguishing features.
