The galaxy presents as a somewhat elongated, disc-like structure with a clearly defined central bulge. The bulge exhibits a yellowish-white hue, suggesting a population of older, less massive stars. Moving outward from the core, a subtle disk structure can be observed. This disk appears mottled, showing a mix of colors suggestive of ongoing star formation. There are hints of blueish regions within the disk, which are indicative of younger, hotter stars and active star-forming regions. The galaxy displays an overall smooth texture with only minor disturbances visible, suggesting it is not undergoing a major merging event or significant gravitational interaction with another galaxy. There is an indication that the galaxy is somewhere between a disk and cigar shape, with the longer axis running from the upper left to lower right of the frame.
