The galaxy appears as a single, centrally condensed object. Its morphology is generally smooth with no obvious spiral arm structure or distinct dust lanes visible in the image. The galaxy exhibits an elliptical shape, showing high degree of roundness with a relatively smooth gradient in luminosity from the core outwards, fading into the background sky. The color profile suggest an older stellar population. The galaxy appears to be isolated, showing no clear signs of interactions or major disturbances with nearby galaxies. The light is mainly concentrated in the center with a relatively compact core, fading towards the outer regions. There are no bright star-forming regions or patchy dust clouds evident.
