The galaxy presents as a relatively compact, elongated structure. Its morphology suggests an edge-on or highly inclined disk galaxy, likely a spiral or lenticular galaxy. The light distribution appears centrally concentrated, with a brighter, somewhat diffuse bulge region. There's a faint suggestion of a disk extending outwards, but the inclination obscures any clear spiral arm structure. The galaxy exhibits a moderately blue hue overall, with some variations in color temperature. The central regions appear slightly redder compared to the outer disk, which presents bluer tones. This could be indicative of older stellar populations in the bulge and ongoing star formation within the disk. No signs of major mergers or significant tidal disturbances are immediately apparent in the galaxy's structure.
