The galaxy presents as a disk galaxy, viewed at a slight angle, though not quite edge-on. A prominent bulge is visible at the center, exhibiting a smooth, yellowish-orange hue. The disk component appears mottled with regions of varying luminosity and color. While a spiral structure is not sharply defined, there are hints of faint, diffuse arms extending outwards from the central bulge. The color distribution suggests a possible gradient, with bluer hues appearing in the outer disk regions, possibly indicative of younger stellar populations and ongoing star formation, and a redder hue closer to the core. There is no obvious evidence of strong tidal disruption or a major merger event, but there are some disturbances. The galaxy appears relatively isolated, with no immediately apparent companion galaxies or signs of a strong interaction.
