The galaxy appears as a relatively smooth, centrally concentrated object. Its morphology is generally elliptical in shape, exhibiting high degree of roundness. There is little evidence of spiral arm structure or a prominent disk. The color profile suggests the presence of an older stellar population, with a reddish hue indicative of evolved stars. No major mergers or significant tidal disturbances are apparent in the immediate vicinity of the galaxy, although there are some minor indications of disturbance present. Overall, the galaxy presents as a passively evolving system with limited ongoing star formation.
