The galaxy presents as a flattened, elongated structure, appearing somewhat cigar-shaped in its overall morphology. A central, concentrated region exhibits a yellowish hue, likely indicating an older stellar population. Extending outward from this central region, a fainter, bluish disk-like component is visible, possibly indicating ongoing or recent star formation. The galaxy does not show any prominent spiral arm structure. The smoothness of the light distribution suggests a relatively evolved system, potentially an elliptical galaxy or a lenticular galaxy viewed edge-on, albeit one with some ongoing star formation. There is no obvious evidence of a major merger event, although a minor tidal disturbance cannot be entirely ruled out based on the faintness of the outer regions. The galaxy is approximately 8.7 kpc in radius.
