The galaxy presents a generally smooth morphology, with a subtle central bulge. Its overall shape appears to be transitioning between round and elliptical, closer to an intermediate form. No distinct spiral arms or bar structures are immediately apparent. There is some subtle texture suggesting minor disturbances in its structure, potentially due to past or ongoing interactions. The color gradient indicates a relatively older stellar population, with a higher concentration of redder stars. There is a faint blue glow in a few areas. The galaxy appears to be relatively isolated with no obvious signs of major merging activity.
