The galaxy presents as a flattened, elongated structure with a discernible central bulge. The morphology suggests a classification towards the elliptical end of the Hubble sequence, with a possibility of being an edge-on spiral galaxy due to the flattened disk. The light distribution is centrally concentrated, becoming fainter towards the edges. The dominant color appears to be yellow-white, indicative of an older stellar population with fewer young, hot stars. There appears to be a minimal presence of distinct spiral arm features or prominent dust lanes. The overall smoothness of the light distribution supports a dominance of evolved stars, suggesting a low star formation rate. There is no obvious evidence of ongoing major mergers or significant tidal disturbances.