The galaxy presents as a moderately bright, elliptical or lenticular-like system, with a smooth, diffuse light distribution. Its core region appears relatively concentrated and luminous, showing a slightly yellowish hue. The outer regions fade gradually into the background sky, suggesting a lack of prominent spiral arms or distinct structural features. There is an absence of intense blue star-forming regions typically associated with younger stellar populations. The galaxy appears to be a relatively isolated system, with no signs of a major ongoing merger or significant tidal disturbance. A subtle asymmetry is detected in the galaxy's overall shape, possibly indicating a minor interaction or past merger event. Based on its color and smooth morphology, the galaxy seems to consist of a primarily older stellar population. 
