The galaxy presents as a relatively smooth, elliptical object. Its core exhibits a concentrated, luminous region, shifting towards a slightly redder hue, indicative of an older stellar population dominating the central region. The surrounding halo appears less defined, fading gradually into the background. There is a hint of bluer light interspersed within the galaxy, possibly indicating some ongoing, albeit subdued, star formation activity. The galaxy displays a generally rounded morphology, without any noticeable distortions suggesting ongoing or recent major merger events. Based on its appearance, it may be classified as an early-type galaxy with a sizable mass, exhibiting a modest rate of star formation.
