The galaxy presents as a somewhat elongated, centrally concentrated object. There is a bright, relatively smooth central bulge, appearing yellowish-white in color, suggesting an older stellar population. Extending outwards from this central region is a fainter, more diffuse disk component. This disk shows hints of spiral structure, though they are not sharply defined. The galaxy's overall color appears to be intermediate, indicating the presence of both young, blue stars and older, redder stars. There appears to be some tidal interaction or perhaps an earlier merger, as evidenced by a slight irregularity in the galaxy's outer regions and an overall disrupted shape. The object seems to have a moderate stellar mass.
