The galaxy presents as a relatively compact structure. It appears predominantly smooth in texture, with a lack of distinct spiral arms or a well-defined disk. The light distribution suggests a centrally concentrated luminosity profile, with the brightest region residing in what appears to be a significant bulge. The galaxy's shape is somewhat elliptical, but leaning towards round. There is no evidence of ongoing major mergers, though hints of minor tidal disturbances or interactions may be present in the outer regions of the galaxy. The overall color is a mix of bluer and redder hues, suggesting a mix of stellar populations.