The galaxy presents as a centrally concentrated object, exhibiting a generally smooth morphology. The light profile appears to gradually decrease in intensity from the core outward, with no distinct spiral arm structures or prominent features readily discernible. The dominant color is a yellowish hue, suggesting an older stellar population and lower levels of ongoing star formation activity. The galaxy exhibits a somewhat rounded shape, showing minimal apparent distortion indicative of potential interactions or merging events. There are no apparent tidal tails, bridges, or other signs of recent or ongoing mergers in the immediate vicinity. The overall appearance suggests a relatively evolved system.
