The galaxy presents as an elliptical or lenticular system, exhibiting a smooth, centrally concentrated light distribution with a noticeable bulge. Its shape is elongated, appearing somewhat cigar-shaped, suggesting it may be an E4-E7 on the Hubble sequence, or possibly an S0 galaxy seen edge-on. 

The galaxy's color is predominantly yellow-orange, indicating a stellar population dominated by older, redder stars with minimal ongoing star formation. There is no visible evidence of spiral arms or significant dust lanes. The galaxy appears relatively isolated, showing no major signs of tidal interaction or recent merger events, though minor disturbances can not be ruled out. The estimated size is approximately 5 kpc in radius.
