The galaxy presents as a relatively compact object, estimated to be approximately 3.7 kpc in effective radius.  Its morphology appears to be disturbed, potentially exhibiting signs of past or ongoing interaction. While a portion of the galaxy appears relatively smooth, there are some features and asymmetries present. There appears to be a small section that might be evidence of tidal tails or disrupted spiral arms. Color gradients are subtle, with a slightly bluer core region transitioning to redder outer regions, suggesting a modest level of ongoing star formation, concentrated towards the center. It appears that there is no substantial major merger occuring, but the minor disturbance from the merging cannot be discounted. Overall, this galaxy appears to be undergoing a slow rate of star formation for a galaxy of its inferred mass.
