The galaxy appears to be a relatively smooth, disk-shaped system, viewed at an oblique angle. It exhibits a central bulge that is bright and yellowish in color, indicating an older stellar population. The disk is elongated and somewhat cigar-shaped, with a subtle color gradient from the central region outwards. There is a faint hint of structure within the disk, potentially suggesting the presence of spiral arms, though these are not well-defined. The disk's color shifts towards redder hues away from the center, possibly due to increased dust extinction or an older stellar population in the outer regions. There are no prominent signs of active star formation, such as bright blue regions or HII regions, and no major merging events are apparent. The galaxy is relatively isolated with no nearby companions visibly interacting with it.
