The galaxy presents a generally smooth morphology, appearing elliptical in shape with a high degree of roundness. There are no strong spiral arm features readily apparent. The light distribution suggests a dominant bulge component, with a centrally concentrated brightness profile. Its color indices indicate the presence of evolved stellar populations, emitting predominantly in the redder wavelengths, although bluer colors are seen in small regions, potentially signaling some pockets of star formation. There is evidence of minor disturbance in the galaxy's structure, possibly from a past or ongoing interaction. Some tidal features may be present at the edge of the galaxy. Overall, the galaxy appears to be a massive system with relatively low star formation activity.
