The galaxy appears as a relatively small, faint, and somewhat diffuse object. It exhibits an overall reddish hue, suggesting a population of older stars and/or significant dust obscuration. The galaxy's morphology is largely smooth, with no immediately obvious spiral arms or a prominent central bulge. However, there appears to be a very faint hint of some irregular structure, potentially indicating a minor disturbance or interaction. There is no clear sign of active star formation regions. Based on the smooth appearance, the galaxy is likely to be an elliptical or lenticular galaxy at a significant distance. 
