The galaxy presents a relatively smooth morphology, exhibiting a notable central bulge that gradually diffuses outwards. The overall shape appears to be elliptical, being more elongated than circular. A faint disk structure is suspected. The core of the galaxy displays a yellowish hue, potentially indicating an older stellar population. The outer regions show hints of bluer colors, suggesting the presence of some younger stars or regions of ongoing star formation, although they are not prominent. There is no distinct evidence of major mergers or significant tidal disturbances. The galaxy appears to be relatively isolated and unperturbed.
