The galaxy presents as a generally smooth, elongated structure. There is a central concentration of light, which seems to be a possible bulge, surrounded by a more diffuse, disk-like component. The galaxy appears flattened with a clear major axis significantly longer than its minor axis. The color gradient within the galaxy suggests a bluer central region possibly indicative of younger stellar populations or active star formation, fading into a redder periphery. The overall form is largely undisturbed, though there might be a slight asymmetry suggesting minor gravitational interaction or internal processes affecting the galaxy's structure. No significant spiral arms or prominent dust lanes are immediately apparent in this image. The galaxy’s disk appears relatively thin, and the absence of significant tidal features suggests it is not undergoing a major merger event.
