The galaxy presents as a relatively smooth, roundish object, exhibiting a concentrated central bulge that graduates into a fainter, more diffuse halo. The core region displays a yellowish-orange hue, suggesting a population of older stars. Fainter greenish-yellow hues are present extending into the halo, though these are more subtle and less prominent. The structure is largely undisturbed, with no obvious signs of major mergers or significant tidal disruptions. There appears to be minimal or no significant ongoing star formation activity based on color.
