This galaxy presents an overall smooth appearance, with a somewhat elliptical morphology. It exhibits a yellowish hue, suggesting a population of older stars. There are indications of tidal disturbances or minor interactions, evidenced by a faint extension or plume-like feature emanating from one side of the galaxy. The galaxy appears relatively isolated, with no obvious major companions or ongoing mergers. The light distribution is centrally concentrated, with a gradual decrease in intensity towards the outer regions. Based on the observed color and morphology, this galaxy is potentially an elliptical or lenticular galaxy at a moderate redshift. Further analysis of the spectral properties is required to determine its precise classification and star formation history.
