The galaxy presents as a somewhat elongated, lenticular structure with a smooth appearance. The light is centrally concentrated, showing a gradual decrease in surface brightness towards the edges. The shape appears significantly elongated, potentially resembling a cigar shape when considering the overall form. There is no clear presence of spiral arms or a well-defined disk.

The galaxy exhibits a redder color, possibly indicative of an older stellar population, lower star formation rate, and higher metallicity within the galaxy. There is a slight irregularity in the light distribution, but overall, the structure does not show any significant disturbances, suggesting a relatively quiescent state. There may be some recent interaction with a neighbor, though it is difficult to definitively determine this from the image.
