The galaxy appears to be a spiral galaxy, seen at a relatively high inclination. A bright central bulge is apparent, exhibiting a yellowish hue suggesting an older stellar population. A fainter, bluer disk surrounds the bulge, its color gradient possibly indicating ongoing star formation in the outer regions. The galaxy's disk is not perfectly symmetrical; there is a slight warping or disturbance visible on the edges, potentially hinting at tidal interactions with another galaxy, although no companion galaxy is immediately apparent in this field of view. The overall morphology of the galaxy suggests an intermediate spiral type, between Sa and Sb.
