The galaxy appears as a relatively compact object, exhibiting a predominantly smooth morphology. It is elongated in shape, suggesting a possible elliptical or lenticular classification. The central region displays a bright, concentrated luminosity, potentially indicative of an active galactic nucleus or a dense stellar population. The color profile appears blue, which could signify ongoing star formation, although this should be confirmed by spectroscopic analysis. There is no obvious spiral arm structure visible in this image, nor are there any signs of strong tidal distortions or recent major merger events. Based on the degree of observed smoothness, it may represent an evolved system with a relatively quiescent star formation history, although the faint blue color indicates some star formation may still be present.
