The galaxy presents as a disk-shaped structure, elongated along a major axis with an approximate ratio of 5:2. The central region exhibits a bright, concentrated core, likely indicating a high stellar density or the presence of an active galactic nucleus, appearing orange in color. The spiral arms are difficult to distinguish. There is a smooth gradient transitioning from the bright core to the outer edges. The galaxy exhibits a color gradient; the central region shows a more red appearance, possibly suggesting an older stellar population and/or dust obscuration, while the outer disk has a bluer color, possibly indicating ongoing star formation. The overall structure appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions.
