The galaxy presents a predominantly smooth morphology. The light distribution appears centrally concentrated, exhibiting a relatively round shape. There is little evidence of spiral arms or a prominent disk structure. The galaxy appears to be relatively isolated, without strong indications of ongoing major mergers or significant tidal disturbances, although there is some slight distortion visible. The color is somewhat red, suggesting an older stellar population with diminished star formation activity. The galaxy has a measured angular size, implying a physical extent of a few kiloparsecs.
