The galaxy presents a generally elliptical morphology. Its color profile is dominated by yellow hues, possibly indicating an older stellar population with a lower rate of ongoing star formation. The light distribution appears relatively smooth, with no distinct spiral arm structures or prominent dust lanes readily apparent. There's a subtle, but definite, irregular feature in the galaxy's shape, possibly indicative of tidal interactions, with a more diffuse outer region. The galaxy's light profile indicates that the core of the galaxy has a high density of stars. There is a secondary concentration of light near the galaxy. There also appears to be a possible connection between them.