The galaxy appears to be an elliptical type, exhibiting a smooth, concentrated light profile. There are indications of a central bulge, and its overall shape is somewhat rounded. The galaxy displays a gradient in color, becoming redder toward its center. There is a suggestion of some minor morphological disturbance, potentially indicating a past or ongoing interaction, however, there is no distinct merging event visible, and no clear evidence of spiral arm structure. The galaxy's overall color suggests a population of older stars, implying a relatively low star formation rate at its current epoch.
