The galaxy presents as a somewhat diffuse elliptical form. The central region exhibits a significantly higher luminosity, suggesting a dense stellar population or possibly an active galactic nucleus. The galaxy appears to have a generally smooth structure with the suggestion of some underlying disk-like morphology. Its color indices indicate the presence of an older stellar population. The galaxy is moderately massive, exhibiting a moderate star formation rate, which is slightly suppressed for its mass, implying a gradual transition towards a quiescent state. There are some hints of minor disturbances in the outer regions, possibly due to a past minor merger event or tidal interaction.
