The observed galaxy appears to be an edge-on spiral galaxy, exhibiting a prominent disk structure oriented nearly perpendicular to our line of sight. The central region displays a notable bulge, appearing smooth and rounded. The disk itself shows a relatively uniform color profile and appears to be relatively thin. Little if any patchiness or discrete spiral arm structure is discernible, possibly indicating a lack of significant current star formation. The galaxy exhibits an overall reddish-yellow hue, consistent with a population of older stars. There are hints of minor dust lane features associated with the disk. The system does not show any obvious signs of major mergers or tidal disturbances, though very slight irregularities could indicate a possible minor interaction in the past.
