The galaxy presents as a relatively smooth, centrally concentrated object. Its light profile suggests a dominant bulge component, with a gradual decline in surface brightness outward from the nucleus. There is little evidence of spiral arm structure or significant dust lanes in the image, pointing towards a possible early-type classification. The shape appears slightly elliptical, with the major axis exhibiting a subtle tilt. The color profile indicates a redder hue, consistent with a population of older stars, and it is likely a massive galaxy. There is no strong evidence of recent or ongoing major mergers. Overall, the galaxy appears to be a well-formed elliptical or lenticular galaxy observed at redshift z~0.115.
