The galaxy presents as a relatively smooth, centrally concentrated system. The light profile appears largely elliptical, with a bright, yellowish core suggestive of an older stellar population dominating the central regions. There is a subtle color gradient moving outward from the core, with a slightly bluer hue in the outer regions, hinting at the presence of some younger stars or ongoing star formation. There does not appear to be any significant dust obscuration or prominent spiral arm structure. There is a mild distortion in the light profile which could be a minor merger occurring, though the galaxy is mostly undisturbed.
