This galaxy appears to be an elongated, disk-shaped system. The central bulge is characterized by a concentrated, yellowish hue, indicative of an older stellar population. Moving outwards from the bulge, the galaxy exhibits fainter, bluer regions within the disk, suggesting regions of ongoing star formation. The disk itself appears relatively smooth, with only subtle hints of spiral arm structure. Overall, the galaxy presents a morphology that is neither perfectly elliptical nor a well-defined spiral, exhibiting characteristics intermediate between the two. There is no clear evidence of major mergers or tidal disturbances in this image.
