The galaxy presents as a centrally concentrated object with a generally smooth appearance, suggestive of an elliptical morphology or potentially a spiral seen face-on with minimal resolved structure. The central region exhibits a bright, yellowish hue, likely indicating an older stellar population. The galaxy extends outwards with a diffuse halo or envelope, becoming bluer in color at larger radii. This color gradient could be indicative of younger stars forming in the outer regions. There is little evidence of strong spiral arm structure or dust lanes. There may be a faint tidal feature or minor disturbance, but it is difficult to say definitively, if this is an artifact. Overall, the galaxy appears relatively isolated. 
