The galaxy presents as a generally smooth, elliptical object, with a bright, concentrated core that fades into the outer regions. Its shape appears to be moderately elongated, but not excessively so. No spiral arm structures or prominent dust lanes are discernible. There are only a few regions of bluer light that indicate some star formation. The light is more dominated by the redder wavelength, indicating an older stellar population. The galaxy doesn't seem to be undergoing a major merger but might show signs of a minor disturbance or interaction that has not significantly disrupted its overall morphology.