The galaxy presents as a generally smooth object with a slightly elongated morphology. The color profile shows a concentration of redder hues toward the central region, with the outer regions exhibiting bluer tones. This color gradient suggests a possible cessation of star formation in the core, while star formation may still be occurring within the outer regions. There appears to be minor asymmetry in the structure, possibly suggestive of a past or ongoing minor interaction or disturbance, but this requires further investigation. The overall light distribution indicates that it is a relatively bright object. The galaxy exhibits an intermediate roundness, leaning more toward being a rounded shape rather than a cigar shape. The classification as a disk galaxy is difficult to see based on the image, but the bluer tones in the outer regions could indicate spiral arms. Further analysis of multi-band photometric data would be needed to determine the specific morphological type and properties.
