The object appears as a relatively compact galaxy with a seemingly smooth morphology. Its color profile indicates a bluer core region transitioning to yellower outskirts. This color gradient could suggest a central region with ongoing star formation and an older stellar population dominating the outer areas. While no clear spiral arms or a bar structure are observed, there may be some subtle distortions in the galaxy's shape. These asymmetries might point to a past or ongoing minor interaction or merger event. Based on the overall appearance, the galaxy could be classified as an early-type spiral or a lenticular galaxy. Further investigation with higher-resolution imaging and spectral analysis would be needed to confirm its exact morphological classification and the details of any potential interaction history.
