The galaxy presents as an elongated, spindle-shaped structure, indicative of a possible edge-on spiral or an elliptical galaxy. A central bulge region is present, exhibiting a bright, concentrated luminosity. Moving outward from the center, the luminosity gradually diminishes into a fainter, more diffuse halo. The light distribution suggests the absence of prominent spiral arms, or their presence may be obscured by the galaxy's orientation. The overall color appears yellowish-white, potentially indicating an older stellar population. The disk appears relatively thin. There is little to no evidence of active star formation in the visible spectrum. The galaxy has a smooth appearance, hinting at a lack of significant recent merger activity.
