The galaxy presents a roughly elliptical morphology, appearing moderately compact with a concentrated central region. There's a strong central bulge dominating the overall light profile, which gradually fades into a less-defined disk or halo structure. The color distribution across the galaxy indicates potential variations in stellar populations. The central region exhibits a bluish-white hue, suggestive of relatively young, hot stars. The outer regions display a slightly greener tone, which might indicate a population of older, cooler stars, or regions of ongoing star formation. There are potential signs of minor disturbances in the galaxy’s structure, possibly suggestive of tidal interactions or minor merger events, though these are subtle. Overall, it is likely a spiral or lenticular galaxy seen at an angle, with indications of ongoing or recent star forming activity in its central bulge.
