The galaxy appears to be an elliptical galaxy, or possibly a lenticular galaxy seen at a shallow inclination. It presents a generally smooth, centrally concentrated luminosity profile. There's a bright, somewhat diffuse central region, grading outwards into a more extended, fainter halo. The shape is somewhat elongated, leaning towards a cigar shape, but is primarily in between round and elongated. There is no strong evidence of spiral arm structure or a prominent disk, nor any major merging activity. The light distribution suggests an older stellar population, supported by a redder hue in the central region. Star formation is present, but it occurs at a low rate. There is a minor disturbance in the morphology of the galaxy. 
