The galaxy presents an elongated, somewhat cigar-shaped morphology. A central bulge region exhibits a brighter, yellowish hue, suggestive of an older stellar population. Extending from the central bulge are fainter, diffuse regions of bluer light, likely indicating areas of more recent star formation. These extended regions appear somewhat disturbed or irregular, lacking a well-defined spiral arm structure. There is also a hint of dust lanes within the disk, especially in the central regions. Overall, the galaxy appears to be at an intermediate stage of evolution.
