This galaxy exhibits a generally smooth morphology, appearing as a moderately elongated, cigar-shaped structure. A notable feature is the presence of a bright, relatively compact region, potentially indicative of a concentrated central bulge or a region of intense star formation. The color gradients suggest some variation in stellar populations or dust distribution within the galaxy, with bluer hues possibly corresponding to younger, hotter stars. There is some asymmetry, perhaps minor disturbances from another body. Overall, the galaxy presents as a relatively evolved system, potentially undergoing or having undergone significant changes.
