The galaxy appears as a relatively compact object with a moderate degree of central concentration. The color profile suggests a bulge that is slightly more prominent in the redder bands, hinting at an older stellar population. The disk structure appears somewhat irregular, possibly indicating ongoing interactions or internal disturbances. There appears to be a slight asymmetry in the outer regions and tidal tails are not obvious. Overall, it is a galaxy that appears to be moderately evolved, with evidence of ongoing star formation and potentially subtle signs of past or current minor merging activity.
