The galaxy presents as a relatively bright object with a somewhat diffuse appearance. It exhibits an overall elliptical shape, trending toward a more rounded morphology. The light distribution appears smooth, lacking prominent spiral arms or a distinct bar structure. There is a suggestion of some disturbed features within the galaxy, possibly indicating a minor interaction or internal dynamics influencing its shape. A subtle color gradient is observed; the central region appears slightly yellower, indicative of an older stellar population, while the outer regions show bluer tints, suggesting the presence of younger, hotter stars and potential ongoing star formation. While the galaxy's light is concentrated in the central region, it does not show a highly concentrated nucleus, rather the light fades gradually towards the outer regions. There also seems to be ongoing activity in the galaxy.
