The galaxy presents as a flattened, elongated structure, characteristic of an edge-on or highly inclined disk galaxy. The central region exhibits a pronounced bulge, which appears rounded and subtly brighter than the surrounding disk. The disk itself shows hints of obscuration, possibly due to dust lanes, although the image resolution limits detailed observation. The overall color profile suggests a population of older stars with a low to moderate star formation rate, with light tending towards the redder end of the spectrum. The galaxy appears relatively isolated, with no obvious signs of ongoing major mergers or significant tidal disturbances.

