The galaxy appears as a centrally concentrated object with a generally smooth morphology, though there is some subtle indication of a disk-like structure or a slightly irregular shape. The color profile indicates a prominent bulge region dominated by older stellar populations, giving it a yellowish hue. Fainter, bluer colors are present in the outer regions of the galaxy, possibly indicating some ongoing star formation. There is no obvious evidence of a major ongoing merger or significant tidal disturbances. The galaxy seems to be relatively isolated, without the presence of bright companion galaxies. It appears to be a relatively massive system with moderate star formation activity.
