The galaxy presents as a generally smooth, elongated structure. Its morphology appears to be that of a flattened ellipsoid, with the longest axis significantly exceeding the shortest, suggesting a disk-like or cigar-like shape. The color profile of the galaxy shows a slight gradient; the central region is more yellow/white, possibly indicating a higher concentration of older stellar populations. Progressing outward from the center, the disk exhibits a bluish hue, potentially signifying the presence of younger, hotter stars.

The structure appears relatively undisturbed, without significant tidal tails, distortions, or signs of ongoing major mergers. There are no prominent dust lanes or distinct spiral arm features visible in this image. The galaxy seems to be in a relatively quiescent state. It is compact in size, but its structure is still well-resolved.
