The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology appears to be elliptical, exhibiting a high degree of roundness. There is a suggestion of a central bulge, marked by a slightly brighter, more concentrated region towards the core. The galaxy exhibits a yellowish hue, indicative of an older stellar population and a lower rate of on-going star formation. Faint, diffuse light extends outwards from the central region, gradually fading into the background sky. The structure does not present any clear spiral arm features, or exhibit any significant morphological disturbances. Evidence for tidal interactions or ongoing merger events is limited; however, there are slight asymmetries within the outer envelope of the galaxy. These could imply the presence of minor perturbations or past interactions, but high resolution imaging would be required to confirm this.
