The galaxy presents as a generally smooth, elliptical morphology. The central region is characterized by a high surface brightness with a yellowish hue, suggesting a population of older stars. Moving outward, the galaxy transitions to a fainter, slightly bluer halo. There is little evidence of distinct spiral arm structure or prominent dust lanes. The shape appears to be somewhere between round and elliptical. No major disturbances or signs of merging events are readily apparent in the image, though there is a chance there could be very minor tidal disturbances. Based on the color, star formation activity appears to be relatively low.
