The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, bright, and yellowish hue, suggesting a population of older stars. This core smoothly transitions into a more diffuse, bluer outer region, perhaps indicative of more recent star formation, even though the overall star formation rate is not very high. The galaxy appears somewhat elongated, without any obvious spiral arm structure or significant signs of tidal disturbance or ongoing mergers. There might be a very subtle disk-like structure faintly visible, but its overall shape looks in-between an elliptical and a spiral galaxy. There is no evidence of significant dust lanes or major morphological peculiarities, suggesting a relatively quiescent evolutionary state. The object’s roundness is not significant, showing that it is not a perfect spheroid.
