The galaxy presents as an elongated, disk-shaped structure, viewed nearly edge-on. There is a subtle central bulge that appears elongated, possibly with a slightly boxy appearance. The overall color suggests a relatively mature stellar population, with a redder hue indicative of older stars and a lower rate of ongoing star formation. The disk appears relatively smooth with no distinct spiral arms or prominent dust lanes visible at this resolution. There is a slight color gradient from the center to the edge, becoming more orange in the middle. No signs of major mergers or strong tidal disturbances are readily apparent.
