The galaxy presents an elliptical morphology, appearing elongated with a cigar-like shape. It exhibits a smooth texture, lacking distinct spiral arms or prominent dust lanes. The central region displays a concentrated, bright yellowish-white core, suggesting a significant population of older stars. The outer regions gradually fade into a fainter, diffuse halo, with a subtle reddish hue. There appears to be no significant evidence of tidal disturbances or ongoing major merging events. The overall color profile indicates a relatively low rate of star formation and a dominant population of evolved stellar populations.
