The galaxy presents a generally smooth morphology, with a high probability of being categorized as such. It exhibits a central bulge, approximately circular in appearance, with a slight elongation. A faint, disk-like structure is potentially present, though not sharply defined. The color profile shows a distinct central region, indicative of an older stellar population, with a relatively redder hue. There appears to be some dust absorption present within the galaxy's disk. There is no strong evidence of ongoing major merging activity, but there is a slight visual disturbance.
