The galaxy presents as a single, fairly well-defined luminous body with a generally elliptical morphology. The light profile appears smooth and centrally concentrated, lacking any obvious spiral arm structure or distinct features suggestive of active star formation regions. There's a hint of color variation in its emission, with a slightly redder hue towards the outer edges. The roundness suggests a relatively low degree of inclination with respect to our line of sight. The overall appearance is consistent with a quiescent galaxy, possibly an elliptical or S0 type, where star formation is suppressed. There are no visual indications of major tidal disturbances or recent merger events.
