The galaxy presents a generally smooth, elliptical morphology. It appears to be a relatively massive system, exhibiting a concentrated central bulge that transitions smoothly into an extended, diffuse halo. The central bulge is characterized by a yellowish-orange hue, potentially indicative of an older stellar population dominated by evolved stars. The surrounding halo displays a bluer tint, suggesting the presence of younger, hotter stars and regions of ongoing star formation, though at a moderate rate. The galaxy appears largely undisturbed, showing no strong signs of tidal interactions or recent major mergers. However, there might be hints of minor distortions or substructure within the outer regions. Overall, this galaxy appears to be an elliptical system with a considerable stellar mass and hints of recent star formation, possibly driven by minor accretion events.
