The galaxy appears as a centrally concentrated object with a moderate degree of ellipticity. A notable feature is its smooth overall appearance, although a subtle disk-like structure may be present within the galaxy. The central bulge exhibits a yellowish hue, possibly indicative of an older stellar population. The surrounding region has a bluer color, implying the presence of ongoing star formation. There are no strong signs of major mergers or significant tidal disturbances, though there is potential for minor interactions. Overall, this galaxy presents characteristics of a transition type, exhibiting properties intermediate between elliptical and spiral morphologies.
