The galaxy exhibits a generally smooth morphology, appearing somewhat spheroidal. The light distribution is concentrated towards the center, with a gradual decrease in intensity outwards. There is evidence of a secondary, smaller concentration of light situated adjacent to the main body. This could be indicative of tidal interactions with a companion galaxy, however the low resolution makes it difficult to ascertain the presence of distinct tidal features. The colour profile tends towards the redder end, implying an older stellar population and/or significant dust obscuration. There is no clear evidence of spiral arms or a prominent disk structure. Overall, this appears to be a relatively evolved galaxy. 
