The galaxy presents as an elongated, disk-shaped structure, oriented approximately edge-on relative to our line of sight. There's a distinct central bulge, characterized by a concentrated, yellowish-white luminosity, suggesting a substantial population of older stars. The disk itself is significantly fainter, with diffuse, extended arms that span a considerable angular extent. The arms exhibit a subtle bluish tinge, particularly at the edges, indicative of the presence of younger, hotter stars and ongoing star formation. There does not appear to be any clear major disturbance, so this galaxy likely has not merged with another.
