The galaxy presents as a moderately bright object, exhibiting an overall smooth appearance. It is neither perfectly circular nor highly elongated; instead, it appears to be of intermediate ellipticity. While a defined disk structure is not immediately apparent, there may be faint features or disturbances, hinting at a possible past interaction or ongoing internal process.

There is some indication of color variation across the galaxy. The central region appears slightly more concentrated and exhibits a subtly redder hue, suggesting an older stellar population. The outer regions appear bluer. Overall, the galaxy does not appear to be undergoing any major mergers, but the aforementioned hints of disturbances may be linked to a minor interaction.
