This galaxy appears to be a spiral galaxy, viewed at an oblique angle. There is a bright, concentrated central bulge exhibiting a yellow-orange hue, suggestive of an older stellar population. The disk component is visible, extending outwards from the bulge, although its structure is somewhat amorphous. There are hints of spiral arms, but they are not clearly defined, and there is a general smoothness to the galaxy's overall appearance. The color of the disk appears bluer, possibly indicating the presence of younger, hotter stars and ongoing star formation, although at a low rate based on the color. The galaxy's shape is elongated, more akin to an in-between round/cigar shape, likely due to the viewing angle. There's no indication of a major merger or significant tidal disturbances in this image.
