The galaxy appears to be a relatively smooth, elliptical type. Its core exhibits a concentrated, yellowish hue, which may indicate an older stellar population. Moving outwards, there is a gradual decrease in luminosity and a shift toward redder colors. There are no readily identifiable spiral arms or prominent dust lanes. There may be very minor asymmetry but overall the structure is fairly regular and unperturbed, with no visible signs of major mergers or tidal interactions.
