The galaxy presents a generally smooth, round morphology, with minimal evidence of spiral arms or bar structures. The light distribution appears centrally concentrated, exhibiting a radial decrease in surface brightness. The color profile indicates a relatively older stellar population. This galaxy is potentially an elliptical or an early-type spiral galaxy viewed at a high inclination angle, but without more detailed spectroscopic data or higher resolution imaging, it is difficult to determine the exact Hubble type. There is no obvious presence of dust lanes, tidal tails, or other features indicative of recent interactions or mergers.