This galaxy presents a somewhat elliptical morphology, appearing largely smooth in its light distribution. There is a discernible central bulge, slightly elongated and exhibiting a yellowish hue, suggestive of an older stellar population. Extending outwards from the core, we observe a fainter, more diffuse disk, displaying hints of blueish tones. The presence of these bluer tones may indicate regions of younger, hotter stars, potentially areas of ongoing or recent star formation. Overall, there is a lack of any obvious spiral arm structure, and the smoothness suggests a later-type spiral or perhaps even an elliptical galaxy, though the observed bluer regions suggest a stronger star formation rate than would be expected for an elliptical galaxy. There are no apparent signs of any recent major merger events or tidal disturbances.
