The galaxy appears to be a relatively small, low-mass system at a redshift of approximately 0.048. Morphologically, it presents a moderately elongated, irregular shape with a noticeable blue tint, indicative of ongoing star formation. There is evidence of minor disturbances in the galaxy's structure, potentially resulting from past interactions or internal dynamical processes. The central region exhibits a somewhat smoother appearance, possibly indicating a more evolved stellar population. The overall color suggests a relatively young stellar population and active star formation is occurring, although at a modest rate. The system shows a mixture of smooth and featured characteristics, with the smooth component dominating, suggesting a transitionary phase in its evolution.
