The galaxy presents a flattened, disk-like morphology, consistent with a spiral or lenticular galaxy. The orientation is nearly edge-on relative to our line of sight, as evidenced by the elongated appearance. A central bulge is discernible, exhibiting a yellowish-white hue, suggesting a population of older stars. The disk appears bluer and fainter, possibly indicative of younger stellar populations and ongoing star formation. There is no evidence of a strong bar structure. The galaxy's profile suggests a smooth light distribution, with light decreasing radially outwards. There are no distinct spiral arms visible, likely due to the edge-on orientation. The overall color suggests an intermediate age stellar population, not dominated by very old or extremely young stars. There is a notable dust lane obscuring the central regions, further suggesting that this is either a spiral or lenticular galaxy.