The galaxy presents as a concentrated, luminous object, exhibiting a smooth morphology. The light profile suggests a centrally concentrated spheroid with a gradual decrease in luminosity outward. The object appears to be comprised of a generally round form, but some visual irregularity hints to that it may not be a perfect ellipse. The color profile skews towards the redder end of the spectrum, indicative of an older stellar population and a potentially lower rate of active star formation within the galaxy. The galaxy exhibits signs of recent or ongoing merging activity due to its irregular shape. Overall, the galaxy appears to be a fairly massive system.
