The galaxy appears to be a relatively small, disk-shaped system seen at a shallow angle, trending towards edge-on. The light distribution is concentrated toward the center, suggesting a prominent bulge or core. There's a notable color gradient, with the central region appearing whiter or possibly slightly yellowish, which may indicate an older stellar population. Fainter, bluer light extends outwards from the core, which could suggest the presence of younger, hotter stars in the disk. The disk structure appears relatively smooth, and there is no clear evidence of spiral arms or strong disturbances, implying a relatively quiescent state.
