The galaxy appears as a relatively bright object, exhibiting a disk-like morphology oriented nearly edge-on with respect to our line of sight. A prominent central bulge, characterized by a yellowish hue, is visible, suggesting a significant population of older stars. The surrounding disk displays a bluer coloration, indicating the presence of younger, hotter stars and ongoing star formation. The disk structure appears somewhat disturbed, potentially due to minor interactions with nearby galaxies or internal processes. The galaxy is not currently undergoing a major merger. Dust lanes are not clearly discernible within the disk, but some obscuration may be present. The overall structure seems indicative of a spiral or lenticular galaxy with active star formation.
