The galaxy presents a largely smooth morphology, with a high degree of circular symmetry observed in its overall shape. The central region exhibits a bright, concentrated core, surrounded by a fainter, more diffuse halo. There is minimal evidence of spiral arm structure or other prominent features within the disk.

The color gradient suggests a population of older stars dominating the galaxy's stellar content, particularly in the central bulge. Bluer regions may indicate the presence of younger stars or ongoing star formation, although this is not prominently visible.

There is an anomaly present over the top of the galaxy that appears to be a digital artifact. This artifact is likely skewing the color and morphology of the true galaxy, as it is unlikely to be a real object.

Given the smooth morphology and color profile, this galaxy appears to be a likely candidate for an elliptical galaxy. Further spectroscopic analysis is needed to determine its redshift and stellar populations to confirm this classification.