The galaxy presents as a slightly elongated, relatively compact object. Its morphology is predominantly smooth, exhibiting a central concentration of light that fades gradually outwards, suggesting an elliptical or lenticular classification. There appears to be a subtle asymmetry to the light distribution, hinting at a possible minor interaction or disturbance. Its color is predominantly yellowish, with a slightly redder hue, indicating an older stellar population and reduced star formation activity. The galaxy does not show any obvious spiral arm structure or distinct features like dust lanes. There is no clear evidence of a recent or ongoing major merger. Overall, the object seems to be a relatively evolved, quiescent galaxy.
