The galaxy presents as a luminous, centrally concentrated object with an overall smooth morphology. The color profile suggests a dominant population of older stars, exhibiting a yellowish-red hue, especially within the central bulge. The object appears largely spheroidal, showing minimal evidence of a disk structure or spiral arms. There's a subtle elongation to the galaxy, though it is close to round. There are no signs of ongoing major mergers, or significant tidal disturbances. The galaxy's light is consistent with minimal recent star formation.
