The galaxy presents as a moderately bright, centrally concentrated object. There is an ambiguous morphology, making it difficult to definitively classify. The galaxy could be described as being relatively smooth in appearance, with a possible disk structure. There appears to be some irregularity in the outer regions that may be indicative of tidal interactions or past mergers. The galaxy exhibits a color gradient, appearing bluer in some regions compared to the more central regions. The overall color suggests a stellar population consisting of both young, hot stars and older, redder stars. This galaxy also has a low redshift, making it farther away.
