This galaxy presents as a relatively smooth, elliptical morphology. The light distribution is concentrated towards the center, exhibiting a bright, well-defined core indicative of an older stellar population. The galaxy appears to be primarily spheroid-dominated, with minimal visual evidence of spiral arms or significant dust lanes. The elliptical shape is more elongated than circular. It is a moderate-sized galaxy. The galaxy appears to be isolated and not undergoing any major mergers or tidal disturbances. The color of the galaxy suggests that it is not undergoing rapid star formation. The absence of strong blue hues typically associated with younger, hotter stars further supports this conclusion. Overall, the galaxy appears to be a relatively quiescent system.
