The galaxy presents as a relatively smooth, elongated structure, suggesting it may be an elliptical galaxy. The central region exhibits a concentrated, brighter core with a yellowish hue, potentially indicative of an older stellar population. Fainter extensions are observed beyond this central bulge and are possibly a disk structure. These regions have a more bluish tint, suggesting areas of younger, hotter stars, possibly related to ongoing star formation. There also appears to be some sort of minor disturbance going on in this system. Overall, the galaxy appears to be at an intermediate stage of evolution, showing characteristics of both older and younger stellar populations.
