The galaxy appears as a centrally concentrated, luminous object with a generally smooth morphology. It exhibits an elliptical shape, with the major axis oriented approximately diagonally in the image. The core region shows a bright, concentrated emission, likely indicative of a high stellar density. The color profile suggests a dominant population of older stars, appearing more yellow/orange in the central region. Fainter, bluer light extends from the central core toward the outer edges of the galaxy, which could be evidence of more recent star formation. There is no prominent disk structure, spiral arms, or bar. No obvious signs of ongoing major mergers are visible, although slight asymmetries or minor disturbances cannot be entirely ruled out. Overall, this galaxy presents as a relatively evolved system, potentially an elliptical galaxy or a lenticular galaxy with a prominent bulge.
