The galaxy appears to be a relatively compact object. Its morphology suggests it is likely an elliptical galaxy, exhibiting a smooth, rather than spiral structure. The galaxy's overall shape is somewhat rounded, with a slight deviation from a perfect circle, possibly indicating some interaction or internal dynamics. The central region shows a concentration of light, suggesting a bright galactic nucleus. There is a hint of a possible extended halo. The color profile indicates a significant red component, suggestive of an older stellar population and/or substantial dust content. There is no clear evidence of active star formation regions from this image. The lack of prominent tidal features suggests this galaxy is not currently undergoing a major merger.
