This galaxy exhibits an overall elliptical morphology, appearing as a flattened spheroid. The light distribution suggests a centrally concentrated structure with a nucleus that is well defined, with a notable decline in luminosity moving outwards from the galactic center. Some faint arm structures can be vaguely discerned, but there is little to no definition to them.

The galaxy's color profile indicates a relatively red composition. The primary luminosity is in the redder wavelengths, suggestive of an older stellar population. There are bluer tinges in parts of the faint arms which may indicate ongoing or recent star formation. The galaxy appears to be relatively isolated, showing no distinct signs of tidal interaction with other nearby galaxies. Some features suggest that the galaxy may have been formed in a minor merger in the distant past.
